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\title{Space Telescope Imaging Spectrograph Observations of High-Velocity
Interstellar Absorption-Line Profiles in the Carina Nebula\altaffilmark{1}}

\author{Nolan R.\ Walborn}
\affil{Space Telescope Science Institute, 3700 San Martin Drive,
Baltimore, MD 21218; walborn@stsci.edu}
\author{Anthony C.\ Danks}
\affil{Emergent-IT, 1801 McCormick Drive, Suite 280, Largo, MD 20774; Anthony.Danks@emergent-IT.com}
\author{Gladys Vieira}
\affil{Science Systems and Applications, Inc., Code 681, NASA/Goddard 
Space Flight Center, Greenbelt, MD 20771; gvieira@hunin.gsfc.nasa.gov}
\author{Wayne B.\ Landsman}
\affil{Science Systems and Applications, Inc., Code 681, NASA/Goddard 
Space Flight Center, Greenbelt, MD 20771; landsman@mpb.gsfc.nasa.gov}
\vspace{1in}
\centerline{\titlelarge To be published in June 2002 issue of the \emph{ApJS}}
\received{3 October 2001}
\accepted{14 December 2001}
\sluginfo
\vfill
\altaffiltext{1}{\titlelarge Based on observations with the NASA/ESA Hubble 
Space Telescope obtained at the Space Telescope Science Institute, which is 
operated by the Association of Universities for Research in Astronomy, Inc., 
under NASA contract NAS5-26555.}
\begin{abstract}
An atlas of ultraviolet interstellar absorption-line profiles toward four
stars in the Carina Nebula is presented.  The observations have been made
with the Space Telescope Imaging Spectrograph on the Hubble Space
Telescope, with a resolving power of 114,000.  Low-ionization,
high-ionization, and excited-state lines from a wide array of chemical 
species are included.  Extensive measurements of radial velocities,
velocity dispersions, and column densities of individual components in 
these profiles are also given.  The unprecedented capabilities of STIS
reveal many more velocity components than previously known; most of the 
high-velocity components in previous observations with the International 
Ultraviolet Explorer are now resolved into multiple subcomponents, and even 
higher velocities are seen.  The great range of line strengths available 
permits the detection of the low-velocity components in the weakest lines, 
and progressively higher velocities in stronger lines (in which the
low-velocity components become completely blended).  The weak and
high-ionization lines trace global structure in the H~II region, while
the strong low-ionization lines show intricate high-velocity structure
that likely originates relatively near to the O~stars observed.  The extreme 
velocities found in the low-ionization lines toward these four stars are 
$-$388 and +127~km~s$^{-1}$, with 23 to 26 resolved components in each.  
Some components in different stars may be related, but many are different 
in each line of sight.  A remarkably well defined Routly-Spitzer effect is 
found in this region.  Temporal variations toward one star observed twice 
have already been reported.  These measurements will be used in subsequent 
astrophysical analyses to further constrain the origins of the phenomena.
\end{abstract}

%\keywords{ISM: abundances --- ISM: individual (Carina Nebula) --- ISM:
%kinematics and dynamics--- ISM: lines and bands--- ISM: structure --- 
%ultraviolet: ISM}


\section{Introduction}
The interstellar absorption lines toward the O~stars ionizing the Carina
Nebula (NGC~3372) have been known for some time to display some of the
most extreme velocity profiles in the Galaxy.  A complete survey of previous 
work and a description of the intricate interstellar phenomenology in this
region were given recently by Danks et~al.\ (2001), so they need not be
repeated here.  In this paper we present an extensive atlas and
measurements of interstellar-line profiles in our Space Telescope Imaging 
Spectrograph (STIS) observations of four Carina Nebula O~stars.  The high
resolution and signal-to-noise of these data substantially extend previous
knowledge of the phenomenon, revealing even higher velocities and finer
component substructure.  These results provide further evidence of the 
extreme spatial variations in the interstellar profiles over small angular 
distances, and they have revealed large temporal variations in one line of 
sight over 22 months (Danks et~al.\ 2001).  They also yield further information
about the qualitatively different behavior in the low-ionization lines (e.g., 
C~II, Mg~II, Fe~II) on the one hand, and the high-ionization (C~IV, Si~IV,
Al~III) and excited-state lines on the other.  These data and measurements 
should enable significant progress toward a physical understanding of the 
extremely structured interstellar medium in the Carina Nebula.   
\medskip

\section{Observations}
The STIS observations of the four targets in our HST General Observer (GO) 
program No.~7301 were made between 1998 March and 1999 April, as detailed 
in Table~1.  The prior ``early-release'' observations (ERO) of 
CPD~$-59^{\circ}$~2603, which permitted the detection of temporal variations 
in its interstellar profiles by comparison with the later data, were obtained 
by program No.~7137 in 1997 June (Walborn et~al.\ 1998, Danks et~al.\ 2001).    
Three of these O~stars (HD~93205, HDE~303308, and CPD~$-59^{\circ}$~2603)
are located relatively near one another in the northern part of the
Carina Nebula and near $\eta$~Carinae, while the fourth (HD~93222) is
situated in the southern part of the nebula (see the maps and figure shown
by Walborn 1982, 1995, respectively).  This circumstance is relevant to
the comparisons among their interstellar profiles below.\footnote{The
distance to the Carina Nebula adopted here is 2500 pc ($1\arcmin\ = 0.73$~pc
in projection).  A thorough discussion of the distance problem is given
by Walborn (1975).  The principal uncertainty is the value of the ratio
of total-to-selective extinction, $R$, which may vary from star to star.
The adopted distance is an average of spectroscopic determinations from the 
O~stars corresponding to $R$~values of 3 and 4, which is the likely range.}

The data were acquired with the STIS high-resolution echelles E140H in
the far-UV (FUV) and E230H in the near-UV (NUV), and the respective
multi-anode microchannel plate array (MAMA) detector for each of the 
two wavelength regions (Woodgate et~al.\ 1998).  Only one exposure in
each configuration was obtained in the ERO program, as detailed in the
earlier papers, but in the GO program three echelle settings, covering
200--300~\AA\ each, were obtained in each wavelength regime for all
targets except the faintest, CPD~$-59^{\circ}$~2603, for which the
longest NUV exposure had to be omitted.  These settings provide complete
coverage of the FUV region, 1150--1700~\AA\ and (with three settings) 
half of the NUV, 1600--3150~\AA, the latter being selected to cover the
greatest number of interesting interstellar lines.  The exposure details
are given in Table~1; the last column lists the stellar continuum flux at
the central wavelength. 

The entrance apertures were $0\farcs2\times0\farcs09$ in the FUV and
$0\farcs1\times0\farcs09$ in the NUV.  The nominal 2-pixel resolving power of 
these STIS configurations is 114,000 (2.6~km~s$^{-1}$).  The ERO observations
were obtained in the STIS Time-Tag mode, in which the 125~$\mu$s samples
are combined and Doppler compensation for the spacecraft motion is
applied in the post-observation data processing; while the GO observations 
were performed in the Accum mode, with automated onboard Doppler
compensation in effect.  The Doppler correction is made in integer pixels
(1.3~km~s$^{-1}$).  The telluric excited-state O~I lines (Spitzer \& 
Fitzpatrick 1993) shown in Figure~15 are probably resolved due to atmospheric 
motions (Jenkins \& Tripp 2001); our Gaussian fits to these features yielded 
FWHM values from 2.9 to 6.6~km~s$^{-1}$, in agreement with their results.  
The typical signal-to-noise in these data is 40.


\section{Measurements}

Following routine technical processing of the MAMA frames, the first step of 
the scientific data reduction is the removal of the scattered light present 
in the echelle images, which becomes progressively stronger toward shorter 
wavelengths.  If not corrected, the scattered light causes an oversubtraction 
of the background, driving saturated lines negative.  All of the images have 
been corrected for scattered light with an optical model of STIS developed 
by Lindler (1998).  The detector background is subtracted separately from the 
scattered-light correction.  A standard one-dimensional spectral extraction 
is performed, with a slit height of 7~pixels for both FUV and NUV data.  
Next the continuum on each side of a line is defined by selecting smooth 
regions and fitting them with a polynomial usually of order two.  The profiles
are then normalized and a check on the scattered light removal is made by
verifying that the central, saturated part of each line is zero.  Finally, 
overlapping wavelength coverages from adjacent echelle orders are weighted 
by the square of their inverse errors and summed.

A line-fitting program is used to arrive at cloud model parameters, namely 
a heliocentric radial velocity, velocity dispersion,\footnote{The velocity
dispersion $b$ is related to the gas temperature $T$ by $b^2 = (2kT/m) + \xi^2$,
where $\xi$ is the most probable speed of the turbulent motions and $m$ is 
the atomic mass.} and saturation-corrected column density for each of the 
components.  The line-spread function used by the program is the model one 
given in the ST~ScI STIS Instrument Handbook, which has a narrow 
(1.6~km~s$^{-1}$) core, but wings due to the telescope point-spread
function that degrade the spectral resolution.  The program utilizes a 
``Levenberg-Marquardt algorithm'' to create the optimal fit, and it generates 
an error estimate as well as a difference fit for the spectral range.  Fits 
were performed starting with the weaker lines such as Mg~II 1239, 1240~\AA\ 
and Mn~II 2576, 2594, 2606~\AA\, in which the lowest velocity components are 
resolved, and then progressing through more saturated lines such as Mg~I
2852~\AA\ and Fe~II 1608, 2382, 2586, 2600~\AA.  The velocity solutions for
these weaker lines were used as inputs to fit the saturated portions of the 
stronger lines Al~II 1670, Si~II 1526, and O~I 1302~\AA.  In this manner, 
velocity structure for the fits to the saturated portions of the strongest 
low-ionization lines, Mg~II 2796, 2803~\AA\ and C~II, C~II* 1334, 1335~\AA\ 
was built up with confidence.   Whenever possible, the high-ionization
lines were fitted independently, but in some severely blended cases velocities 
derived from low-ionization components had to be adopted.  In general,
radial velocities adopted from other line fits can be recognized by their
zero decimals.  In order to prevent divergence of the fits in the most
blended and saturated portions of the profiles, upper limits to the allowed 
velocity dispersions were fixed at 10~km~s$^{-1}$ for the low-ionization 
lines, and 12~km~s$^{-1}$ for the high-ionization lines.  In a few cases
for which it appeared to be appropriate, lower velocity dispersions were 
fixed to prevent the program from defaulting to the upper limits in blended 
regions; these cases are also generally distinguished by their zero decimals.  
Examples of fits to a low-ionization and a high-ionization profile are shown 
in Figures~1a--b.  

Radial velocities of unblended components are accurate to $\sim1$~km~s$^{-1}$, 
the limiting factors being the thermal stability of STIS, wavelength 
zeropoints, and the dispersion solutions.  Unsaturated column densities have 
typical accuracies of 10\%; those judged to be more uncertain than twice that 
amount are flagged with colons in the data tables.  No measurements are 
reported in cases of blends between two different species, or when there were 
four or more adjacent velocity components within a completely black trough.   


\section{Results}

The intricate interstellar profiles revealed by STIS toward these Carina
Nebula O stars are presented here in an atlas format, while extensive
measurements of individual velocity components are given in the
accompanying tables.  The atlas is arranged as follows.  Two figures for
each star (Figures~2--9) present the low-ionization lines, ordered by 
increasing line strength; the first figure in a pair has four parts, each 
of which is a montage of five line profiles, while the second figure of
the pair shows the highly complex, overlapping C~II, C~II* profiles 
separately.  Then an additional figure for each star (Figures~10--13) 
displays the high-ionization doublets as montages of six lines.  Finally, two 
more figures (Figures~14--15) are montages of two complex but interesting
wavelength regions containing partially overlapping excited-state lines, with 
all four stars shown together in each case.  Tables~2--5 provide measurements 
of heliocentric radial velocities, velocity dispersions, and column densities 
ordered by increasing radial velocity for each star. For a given velocity
component, the chemical species are listed alphabetically, and multiple
lines from the same species are in order of increasing wavelength.  Similar 
(but often not identical) low- and high-ionization component velocities are 
listed together, with a blank line separating the latter from the former.
The tables include measurements of additional lines not shown in the figures.
Vacuum wavelengths are used throughout this paper.

\subsection{CPD~${\bf -59^{\circ}}$~2603}

This star was observed with STIS in both 1997 and 1999; partial analyses
of the results, including large temporal variations in the profiles
between the two epochs, have been presented by Walborn et~al.\ (1998) and
Danks et~al.\ (2001).  In Figures~2a--d, the subset of profiles observed
in 1997 are superposed with dashed lines, while the C~II, C~II* profiles
at the two epochs are shown displaced in Figure~3.  Entries in Table~2 for 
the same velocity component at the two epochs are distinguished by
footnotes; of course, the majority were observed only in 1999 because of
the limited wavelength coverage in 1997.  In the case of the
``69/72~km~s$^{-1}$'' components, measurements are given for only the first 
velocity in 1997 and the second in 1999, since the stronger feature at the 
lower velocity disappeared between the two epochs, and the weaker, higher
velocity one was severely blended at the earlier epoch.  The high-ionization 
interstellar lines in this spectrum are shown in Figure~10, and some 
further excited-state profiles in Figures~14 and 15.  The Si~IV doublet
is shown for both epochs in Fig.~10, but the Al~III is missing because
the grating setting that covers it had to be omitted from the program.

The prior groundbased (Walborn 1982) and IUE (Walborn \& Hesser 1982)
observations had revealed a total of 9 low-ionization interstellar velocity 
components in this line of sight, including 4 with very high velocities.  
The more sensitive STIS data resolve multiple substructure in most of these 
components and detect many new ones, with a total of 25 components between  
$-$233 and +127~km~s$^{-1}$.

Considering first the weaker lines (Fe~II through Mn~II in Figs.~2a--b),
one sees 4~dominant components at $-$38, $-$19, $-$3, and +8~km~s$^{-1}$,
in excellent agreement with measurements of the optical Ca~II and Na~I
profiles (Walborn 1982).  This structure will be seen to be quite similar 
toward all three stars in the northern part of the Carina Nebula, but very 
different toward the star in the southern part.  The two lower velocity 
components likely arise along the $\sim$2500~pc line of sight\footnote{No 
high-velocity interstellar lines due to galactic structure and differential
rotation are expected in this direction (Rickard 1974).  It is likely that
at least some of the interstellar velocity components within about
$\pm$10~km~s$^{-1}$ arise along the general line of sight.  Astrophysical
analysis of some weak, low-velocity, heavy-element lines in Walborn et~al.\
(1998) indicates that they may arise in diffuse clouds near the Sun.} to the 
complex, but the $-$38~km~s$^{-1}$ and possibly the $-$19~km~s$^{-1}$ 
components are related to the global expansion of the H~II region, as inferred 
from comparisons with the double nebular emission lines (Walborn \& Hesser
1975) and the high-ionization absorption lines (Walborn, Heckathorn, \&
Hesser 1984, and below).  Despite the overall similarities, marked
differences occur in the relative strengths of these four velocity 
components among the different species, e.g., the much greater strength of 
the $-$19~km~s$^{-1}$ in the Mg~II and Mn~II lines, and of the +8~km~s$^{-1}$ 
in Cl~I.  When analyzed quantitatively, these differences will provide
valuable diagnostics of the relative ionizations, abundances, and depletions
in the material giving rise to the various components, and ultimately clues 
to their sites of origin. 

The S~II lines (Fig.~2b) are the most ``useless,'' since the low- and
intermediate-velocity components have become completely blended, while
the high-velocity ones are not yet well detected.  The latter appear
clearly in Mg~I (Fig.~2c) and strengthen to their maximum intensities in
Mg~II (Fig.~2d) and C~II (Fig.~3).  Again, despite the similarities in
the profiles of the strong lines, significant differences can be seen in
the relative strengths of certain components among the different species,
e.g., the weaker $-$166~km~s$^{-1}$ and stronger +61~km~s$^{-1}$ in O~I
compared to adjacent profiles.  As before, quantitative analyses of these
effects will provide physical insights into the formation and origins of
the different components.  The C~II, C~II* profiles offer additional
interesting information, namely the disappearance of the +69~km~s$^{-1}$
component and changes in the strengths of other components between the two 
epochs, confirming the Mg~II variations reported by Danks et~al.\ (2001); and 
the resolution of the weaker C~II* 1335.663~\AA\ line at +98~km~s$^{-1}$.  
Both C~II* lines are entered in Table~2 at the latter velocity to record their 
presence, although the fitting program assumes identical parameters for them. 

As known from previous work, the dominant components of the
high-ionization lines (Figure~10) are at intermediate negative velocities, 
corresponding to the global expansion of the H~II region (Walborn et~al.\
1984).  Two principal components at $-$44 and $-$30~km~s$^{-1}$ have been
fitted to the CPD~$-59^{\circ}$~2603 profiles, based on the appearance of
the C~IV lines; the average of those velocities is similar to a dominant
component resolved in the weak low-ionization lines, which is likely related.  
The features near zero velocity may provide a rare opportunity to investigate 
high-ionization lines along the general Galactic-disk line of sight, far
from the hot stars against which they are observed, since H~II region
material at those velocities should be mostly behind the stars.  There is 
clearly high-velocity structure in the high-ionization lines, but it is
weaker and less well defined than in the low-ionization lines.  The
fitted high-ionization velocities tend to be similar to or more negative
than those of the most similar low-ionization components (Table~2), which 
may or may not be significant at this early stage of the analysis.  Although
the very strong excited-state line of Si~II* 1264.7~\AA\ (Figure~14) has 
well-marked high-velocity features, all of the excited-state lines (see 
Figure~15 as well) share the property of the high-ionization lines that
their dominant components are at the intermediate negative velocities.
Note the strong telluric components of O~I* and O~I** in Fig.~15 (Spitzer
\& Fitzpatrick 1993; Jenkins \& Tripp 2001).

\subsection{HD~93205}     

The low-ionization interstellar profiles toward this star are displayed
in Figures~4a--d and 5, the high-ionization lines in Figure~11, and some
further excited-state lines in Figures~14 and 15.  The corresponding 
measurements are listed in Table~3.  In this and the subsequent data tables,
measurements of the same lines from different (overlapping) images are 
specified by the central wavelengths of the latter in footnotes.   

A total of 6 low-ionization velocity components, including two with very
high velocities, were detected in the prior groundbased and IUE studies.
The STIS data reveal 23 low-ionization components ranging in velocity from
$-$142 to +118~km~s$^{-1}$.  Particularly noteworthy are the 
extreme negative velocity, which corresponds to a quite strong component
in the more intense lines that was not detected in the earlier work, and
the resolution of the former $-$89~km~s$^{-1}$ feature into 3~strong
subcomponents (Figs.~4c--d).

The velocity structure in the weak lines at low and intermediate velocities 
(Figs.~4a--b) is virtually identical to that in CPD~$-59^{\circ}$~2603,
demonstrating that it corresponds to global structure in the H~II region,
as well as the Galactic-disk line of sight.  Unlike CPD~$-59^{\circ}$~2603,
however, HD~93205 has some high-velocity components already well detected in
Mn~II and S~II (Fig.~4b), showing that they are intrinsically stronger
than those toward the other star.

As in all cases, the strongest high-ionization (Fig.~11) and excited-state  
(Figs.~14 and 15) components are at an intermediate negative velocity,
$-$35~km~s$^{-1}$ toward HD~93205, corresponding to the blue-shifted near
side of the expanding H~II region.  There is a major low-ionization
component at an identical velocity, which likely has the same origin.
The behavior of the other principal components in the high-ionization lines
is interesting: the one at $-$61~km~s$^{-1}$ is proportional to the
degree of ionization (strongest in C~IV), while the blend of the $-$3 and
+8~km~s$^{-1}$ components is inversely proportional (strongest in Al~III).
This behavior is consistent with an origin of the high negative-velocity
feature within the H~II region, but the low-velocity features along the
Galactic-disk line of sight as predicted on morphological grounds above. 

\subsection{HDE~303308}

This star, located 1\arcmin\ north of $\eta$~Carinae, has the most
heavily blended interstellar profiles in the present sample.  The
low-ionization lines are shown in Figures~6a--d and 7, the high-ionization 
lines in Figure~12, and further excited-state lines in Figures~14 and 15.  
The measurements are given in Table~4.

The groundbased and IUE studies resolved 11 low-ionization velocity
components toward HDE~303308, of which 7 had very high velocities.  The
fact that so many high-velocity components are visible in the relatively
weak Ca~II lines is directly related to the heavy blending encountered in
the strong UV lines.  In the STIS data, 24 low-ionization components
between $-$175 and +98~km~s$^{-1}$ are distinguished, although many of
the measurements are relatively uncertain due to the blending.

The weak, low to intermediate-velocity lines (Figs.~6a--b) have essentially
the same structure as in CPD~$-59^{\circ}$~2603 and HD~93205, although
the principal components are more blended and hence less distinct.  Also,
the component at $-19$ to $-$18~km~s$^{-1}$ in the other two stars, that
becomes relatively stronger in Mg~II and Mn~II, has shifted to
$-24$~km~s$^{-1}$ in HDE~303308, thus becoming more blended with the next
higher negative-velocity one.  Also unlike the other two stars, HDE~303308 
has significant absorption in Cl~I at intermediate negative velocities.
As in HD~93205, some very high-velocity features are already well defined
in Mn~II and S~II (Fig.~6b).  In the strongest lines, Mg~II and C~II, CII* 
(Figs.~6d and~7) there are no unblended components except for the weak 
new ones at the extreme velocities of $-$133 and $-$175~km~s$^{-1}$.

Unlike in HD~93205, the high-ionization component at $-$60~km~s$^{-1}$ and
another at $-$78~km~s$^{-1}$ toward HDE~303308 (Fig.~12) are strongest at
the intermediate ionization of Si~IV.  On the other hand, the blended
$-$3 and +6~km~s$^{-1}$ components are strongest in Al~III, analogously
to HD~93205.  

\subsection{HD~93222}

HD~93222 is located in the southern part of the Carina Nebula, 20--25\arcmin\ 
from the other three stars, and it holds the interstellar speed record in
this region, with a strong component in Mg~II and C~II at $-$350~km~s$^{-1}$
found in the IUE data (Walborn \& Hesser 1982).  Some apparent
relationships to diffuse X-ray emission and near-UV nebulosity were
pointed out in that paper.  The STIS observations of the low-ionization
interstellar lines are displayed in Figures~8a--d and~9, the
high-ionization lines in Figure~13, and some further excited-state lines
in Figures~14 and 15.  The measurements are listed in Table~5.

Five interstellar low-ionization velocity components were resolved in the 
groundbased and IUE work, including two with very high velocities.  The
high-ionization lines toward this star seemed to show more discrete
velocity structure than those toward the other stars in the IUE data,
although the S/N was modest (Walborn et~al.\ 1984).  The STIS data resolve
26~low-ionization velocity components between $-$388 and +93~km~s$^{-1}$, 
and they amply confirm the interpretation of the high-ionization profiles 
in the IUE data.  Remarkably, the $-$350~km~s$^{-1}$ feature breaks up into 
6~subcomponents, with the strongest at $-$372~km~s$^{-1}$; some of them are 
clearly present in C~IV as well.

The profiles of the weak, low-velocity lines (Figs.~8a--b) are
qualitatively different from those toward the other three stars in the
northern part of the nebula, showing that the global and Galactic
line-of-sight structures are different toward the southern part.  The
strongest component is at $-$23~km~s$^{-1}$, with two additional principal 
components at $-$6 and +6~km~s$^{-1}$, the latter itself likely composite.  
Cl~I has a well resolved double structure corresponding to the last two 
velocities, but the +6~km~s$^{-1}$ component does not appear composite
in this line.  Intricate higher velocity structure first appears in Si~II 
and S~II (Fig.~8b) and develops progressively in the stronger lines 
(Figs.~8c--d), including the multiple extreme negative-velocity feature.
The latter is relatively weaker in O~I, however; note also that this
feature from C~II* blends with the shortward edge of the black trough at 
lower velocities in C~II (Fig.~9), as was already shown by the IUE data.

The high-ionization interstellar lines toward HD~93222 (Fig.~13) show 
stronger discrete velocity structure than those toward the other stars.  
There are five major components, at $-$20, $-$34, $-$48, $-$66, and
$-$83~km~s$^{-1}$.  All of them have close counterparts in the
low-ionization lines.  Curiously, unlike in the other stars, none of them 
is completely black in C~IV, in which the $-$66~km~s$^{-1}$ is the
strongest.  In contrast, the $-$20~km~s$^{-1}$ component is dominant (and
black) in Si~IV and Al~III.  There appears to be a correlation between
absolute velocity and ionization among all of the high-ionization
components.  As in HD~93205 and HDE~303308, one at +6~km~s$^{-1}$,
presumably from the Galactic line of sight, is strongest in Al~III;
components at +17, $-$20, $-$34, and $-$48~km~s$^{-1}$ are strongest in 
Si~IV; while those at $-$66 and $-$83~km~s$^{-1}$ are strongest in C~IV. 
As already mentioned, some of the extreme negative-velocity subcomponents
are also present in C~IV.  The principal components in the excited-state
lines (Figs.~14 and 15) are at $-$24--25~km~s$^{-1}$, similarly to those in
Si~IV and  Al~III, and to the strongest component in the low-ionization lines. 

\subsection{Collation of Velocity Components among Stars}

Table~6 compares the low- and high-ionization velocity components observed
toward the four stars, with CPD~$-59^{\circ}$~2603 as the reference.  The
occurrence of identical velocities in low- and high-ionization components
generally indicates that the latter were adopted from the former to
resolve ambiguous, blended profiles.  While many velocity components are 
unique to each star, several similar velocities are seen to occur in some or 
all of them.  The most notable of the latter are at approximately $-$100,
$-$90, $-$65, $-$35, $-$20, $-$5, +5, +20, +35, +65, +90, and +100~km~s$^{-1}$.
The apparent symmetry between negative and positive velocities is
illusory, however, because these are heliocentric values; they must be
corrected by +14~km~s$^{-1}$ to the Carina Nebula rest frame
as defined by the double nebular emission lines (Walborn \& Hesser 1975).
The two lowest (absolute) velocities likely correspond primarily to the full 
$\sim$2500~pc line of sight to the Carina Nebula, and the black troughs from 
about $-$50 to +30~km~s$^{-1}$ in the intermediate-strength, low-ionization 
lines are very similar in all the stars.  The components near $-$35~km~s$^{-1}$ 
likely correspond to the near side of the globally expanding H~II region, 
because they coincide with the blueward component of the double nebular 
emission lines and dominate the high-ionization absorption profiles
(except in HD~93222 in the southern part of the nebula).  There 
is the interesting possibility that the +69~km~s$^{-1}$ component that
disappeared between 1997 and 1999 in CPD~$-59^{\circ}$~2603 may be
present in HD~93205, although it is not possible to rule out a chance 
velocity coincidence between the two stars.  It will be difficult to
establish coherent high-velocity physical structures among the stars
because of the rapid spatial variations in the profiles, the sparse
angular sampling, the unknown (small) distribution in depth of the stars,
and the possibility that the radial velocities of any such structures would
vary from star to star due to acceleration and projection effects.    

\section{Discussion}

This paper presents an atlas of profiles, measurements of individual
velocity components, and some morphological inferences from the complex 
interstellar absorption lines toward four O~stars in the Carina
Nebula, as observed with HST/STIS.  The principal results are the much 
larger numbers of velocity components, somewhat higher velocities, and 
especially the substructure found in most of the high-velocity components, 
in comparison with previous groundbased and IUE investigations.
In addition, temporal variations were discovered in a number of
velocity components toward one star observed at two epochs.  These results 
provide vital new information about the physical origins of the phenomena
and demonstrate the futility of quantitative analyses of the earlier data. 

These new data provide the basis for further astrophysical studies
directed toward improved understanding of the various velocity regimes in
the interstellar profiles.  Specifically, the hypotheses that the highest
velocity features in the low-ionization lines arise from an interaction
of the stellar winds with surrounding interstellar material, and that the
dominant components in the high-ionization and excited-state lines
correspond to the global expansion of the H~II region, will be addressed
by these studies.  Additionally, Danks et~al.\ (2001) pointed out the
morphological similarity between the interstellar profiles toward  
CPD~$-59^{\circ}$~2603 and a QSO narrow-line system (see also Bond et~al.\ 
2001).  Quantitative comparisons between the Carina Nebula interstellar 
profiles and an array of QSO systems observed with comparable resolution, 
as well as a search for rapid temporal variations in the latter, will probe 
whether some of the QSO systems might arise in intervening starburst regions.

As a first astrophysical interpellation of the data, Figures~16a--b 
show plots of column-density ratios as a function of local radial velocity 
(corrected by +14~km~s$^{-1}$ from heliocentric; Walborn \& Hesser 1975) for
Mg~II/Fe~II and Si~II/Fe~II, following Welty et~al.\ (1997).  All of these
ions have similar ionization potentials and are dominant.  Only the best 
quality column densities have been used for these calculations, i.e., very 
weak or badly saturated components have been omitted, and means of the same 
velocity component in different lines from the same species in a given star 
have been taken when possible.  The uncertainties of the points in 
Figs.~16a--b range from 0.05 to 0.1~dex, as estimated from propagation of 
the column-density errors to the ratios, with the smaller uncertainties 
corresponding to means of components.  Since Fe is more heavily depleted than 
Mg or Si, these plots show the Routly-Spitzer (1952) effect, with less 
depletion and hence smaller ratios at the higher velocities.  For comparison,
standard ratios from Savage \& Sembach (1996) are indicated at the right
for conditions ranging from the cool Galactic disk (highest depletions)
to solar abundances (undepleted gas phase).  The ranges of depletions in
the Carina Nebula are in reasonable agreement with the standard values;
the somewhat more extreme values in Mg~II/Fe~II may be due to measurement
uncertainties in these strong lines.  Because of the large number of 
components, the velocity range over which the lifting of the depletion 
occurs is exceptionally well defined, i.e., within $\pm$100~km~s$^{-1}$.  
An analogous effect was shown in Na~I/Ca~II by Walborn (1982, Fig.~25).  
It is interesting that this effect occurs in the Carina Nebula high-velocity 
material, despite the quite different environment from those in which it 
is generally observed.  

Figure~17 shows the C~IV/Si~IV column-density ratios, which diagnose 
ionization mechanisms (e.g., Franco \& Savage 1982), as a function of local 
radial velocity.  All available ratios have been plotted here; the uncertainty 
of most points in Fig.~17, estimated from propagation of errors and comparison 
between doublet members, is $\sim$0.1~dex, but the three lowest points and 
one for HDE~303308 at $-$23~km~s$^{-1}$, log ratio 0.03 correspond to 
saturated components and have errors of at least 0.2~dex.  Walborn et~al.\ 
(1984) found low values of the ratio in Carina Nebula intermediate-velocity 
components, indicative of photoionization and consistent with their 
interpretation as the near side of the globally expanding H~II region; and 
higher values in high-velocity components, implying the presence of X-ray 
and/or collisional ionization.  The present results in Fig.~17 are in good 
agreement with the earlier ones.  The observed ratios nicely span the
typical range of the three ionization mechanisms, with the lowest values
corresponding to photoionization at intermediate velocities.  The envelope 
curve of the distribution suggests a gradual appearance of the other 
mechanisms as a function of increasing absolute velocity, but the curve is 
``filled in,'' implying an overlap of mechanisms at intermediate radial 
velocities.  These results will be further discussed in future papers,
including the possibility of velocity dispersions larger than the upper 
limit of 12~km~s$^{-1}$ adopted in the present fits, for lines in the 
collisional regime.

Despite the extensive presentation here, it does not exhaust the
information content of the data.  In particular, they contain rich sets
of (overlapping) C~I, C~I*, C~I** profiles and absorption lines from
numerous transitions of CO, which remain to be measured and analyzed.

Further STIS observations of these and other stars in the Carina Nebula
will also be essential to fully characterize the phenomena.  The one case
observed at two epochs revealed large temporal variations.  Additional
epochs for this star and the other three observed here will support
statistical inferences about the incidence and timescales of the
variations, as well as the sizes, transverse velocities, and distances
from the stars of the discrete absorbing structures.  Furthermore, the
groundbased and IUE work demonstrated rapid spatial variations of the
interstellar profiles, with some velocity components possibly in common 
but many completely different between pairs of stars separated by small
angular distances.  In view of the far greater complexity of the profiles
revealed by STIS, other stars near those discussed here must be similarly
observed to constrain the spatial extents of the absorbing structures,
in depth as well as across the line of sight.  Excellent candidates near
the present targets exist, namely HD~93204 (only 20\arcsec\ or 0.24~pc in
projection from HD~93205), CPD~$-59^{\circ}$~2600, HD~93130, and HD~93146 
(the last two in the southern part of the nebula).  These additional 
observations need not cover the full range of wavelengths observed here, but 
just a few lines of intermediate and large intensities to define the variations.
  
\acknowledgments
Support for this work was provided by NASA through grants GO-7301-96A from 
the Space Telescope Science Institute, which is operated by AURA, Inc., under
contract NAS 5-26555; and a grant to the STIS Instrument Definition Team (ACD).
We thank the anonymous referee for several useful and courteous suggestions.

\begin{references}
\reference{} Bond, N.~A., Churchill, C.~W., Charlton, J.~C., \& Vogt, S.~S.
   2001, \apj, 562, 641
\reference{} Danks, A.~C., Walborn, N.~R., Vieira, G., Landsman, W.~B., Gales, J.,
   \& Garc\'{\i}a, B. 2001, \apj, 547, L155
\reference{} Franco, J.\ \& Savage, B.~D. 1982, \apj, 255, 541
\reference{} Jenkins, E.~B.\ \& Tripp, T.~M. 2001, \apjs, 137, 297
\reference{} Lindler, D. 1998, CALSTIS Reference Guide (Version~5.1), 
   http://hires.gsfc.nasa.gov/stis/ software/software.html
\reference{} Rickard, J.~J. 1974, \aap, 31, 47
\reference{} Routly, P.~M.\ \& Spitzer, L., Jr. 1952, \apj, 115, 227
\reference{} Savage, B.~D.\ \& Sembach, K.~R. 1996, \araa, 34, 279
\reference{} Spitzer, L., Jr., \& Fitzpatrick, E.~L. 1993, \apj, 409, 299
\reference{} Walborn, N.~R. 1982, \apjs, 48, 145
\reference{} ----- 1995, RevMexAA (Ser.\ Conf.), 2, 51
\reference{} Walborn, N.~R., et~al. 1998, \apj, 492, L169
\reference{} Walborn, N.~R., Heckathorn, J.~N., \& Hesser, J.~E. 1984, \apj, 276,  
   524
\reference{} Walborn, N.~R.\ \& Hesser, J.~E. 1975, \apj, 199, 535
\reference{} ----- 1982, \apj, 252, 156
\reference{} Welty, D.~E., Lauroesch, J.~T., Blades, J.~C., Hobbs, L.~M., \& 
   York, D.~G. 1997, \apj, 489, 672
\reference{} Woodgate, B.~E., et~al. 1998, \pasp, 110, 1183
\end{references}

\newpage
\begin{landscape}
\begin{figure}
\centering
\includegraphics[height=\textheight,angle=90]{newfig1a.eps}
\caption{a) Illustration of the profile fitting for the low-ionization line
Mg~II 2803~\AA\ toward CPD~$-59^{\circ}$~2603 in 1997.  The lower panel
shows the residuals.
\label{fig1}}
\end{figure}
\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=\textheight,angle=90]{newfig1b.eps}
%\centerline{\psfig{figure=fig1b.eps,height=5.5in,angle=90}}
\caption{b) Same for the high-ionization line C~IV 1548~\AA\
toward CPD~$-59^{\circ}$~2603 (in 1999).
\label{fig1}}
\end{figure}
\end{landscape}


\begin{figure}
\centering
\includegraphics[height=8in]{fig2a.eps}
\caption{a) Sequence of rectified, low-ionization interstellar-line profiles 
toward CPD~$-59^{\circ}$~2603, ordered by increasing strength.  In this
and all subsequent plots, the data have been smoothed by 3~pixels.
The heliocentric radial velocities [km~s$^{-1}$] of all discrete components 
measured in the low-ionization lines are marked at the top.  For lines
observed at both epochs, the 1997 profiles are superposed with dashed
lines.  Other species present in a given panel are identified.  The
sequence continues in the next three figures.  
\label{fig2}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig2b.eps}
\caption{b) {\it Continuation.}
\label{fig2}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig2c.eps}
\caption{c) {\it Continuation.}
\label{fig2}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig2d.eps}
\caption{d) {\it Continuation.}
\label{fig2}}
\end{figure}

\begin{figure}
\centering
\includegraphics[height=8in]{fig3.eps}
\caption{Rectified profiles of the very strong, partially overlapped
interstellar C~II, C~II* lines toward CPD~$-59^{\circ}$~2603 at both
epochs, which are displaced by 0.5 continuum units.  Note the disappearance 
of the +69~km~s$^{-1}$ component between the two epochs, and the
resolution of the weaker of the two C~II* lines at +98~km~s$^{-1}$
(denoted as ``98w'').
\label{fig3}}
\end{figure}

\begin{figure}
\centering
\includegraphics[height=8in]{fig4a.eps}
\caption{a) Sequence of low-ionization interstellar-line profiles toward
HD~93205.  The sequence continues in the next three figures.
\label{fig4}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig4b.eps}
\caption{b) {\it Continuation.}
\label{fig4}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig4c.eps}
\caption{c) {\it Continuation.}
\label{fig4}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig4d.eps}
\caption{d) {\it Continuation.}
\label{fig4}}
\end{figure}

\clearpage

\begin{figure}
\centering
\includegraphics[width=5.5in]{fig5.eps}
\caption{The C~II, C~II* interstellar lines toward HD~93205.
\label{fig5}}
\end{figure}

\begin{figure}
\centering
\includegraphics[height=8in]{fig6a.eps}
\caption{a) Sequence of low-ionization interstellar-line profiles toward
HDE~303308.  The sequence continues in the next three figures.
\label{fig6}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig6b.eps}
\caption{b) {\it Continuation.}
\label{fig6}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig6c.eps}
\caption{c) {\it Continuation.}
\label{fig6}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig6d.eps}
\caption{d) {\it Continuation.}
\label{fig6}}
\end{figure}

\begin{figure}
\centering
\includegraphics[width=5.5in]{fig7.eps}
\caption{The C~II, C~II* interstellar lines toward HDE~303308.
\label{fig7}}
\end{figure}

\begin{figure}
\centering
\includegraphics[height=8in]{fig8a.eps}
\caption{a) Sequence of low-ionization interstellar-line profiles toward
HD~93222.  The sequence continues in the next three figures.
\label{fig8}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig8b.eps}
\caption{b) {\it Continuation.}
\label{fig8}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig8c.eps}
\caption{c) {\it Continuation.}
\label{fig8}}
\end{figure}

\addtocounter{figure}{-1}
\begin{figure}
\centering
\includegraphics[height=8in]{fig8d.eps}
\caption{d) {\it Continuation.}
\label{fig8}}
\end{figure}

\begin{figure}
\centering
\includegraphics[width=5.5in]{fig9.eps}
\caption{The C~II, C~II* interstellar lines toward HD~93222.  Note that
the C~II* features at $-$350 to $-$388~km~s$^{-1}$ are blended at the
shortward edge of the black trough in C~II.
\label{fig9}}
\end{figure}

\clearpage

\begin{figure}
\centering
\includegraphics[height=8in]{fig10.eps}
\caption{Rectified, high-ionization interstellar-line profiles toward
CPD~$-59^{\circ}$~2603.  The heliocentric radial velocities [km~s$^{-1}$] of 
the fitted components are marked at the top, and extraneous species in a given 
panel are identified.  The Si~IV lines were covered at both epochs; the 1997 
data are so marked.  (The Al~III lines were not observed in this line of sight.)
\label{fig10}}
\end{figure}

\begin{figure}
\centering
\includegraphics[height=8in]{fig11.eps}
\caption{High-ionization interstellar-line profiles toward HD~93205.
\label{fig11}}
\end{figure}

\begin{figure}
\centering
\includegraphics[height=8in]{fig12.eps}
\caption{High-ionization interstellar-line profiles toward HDE~303308.
\label{fig12}}
\end{figure}

\begin{figure}
\centering
\includegraphics[height=8in]{fig13.eps}
\caption{High-ionization interstellar-line profiles toward HD~93222.
\label{fig13}}
\end{figure}

\begin{figure}
\centering
\includegraphics[width=5.5in]{fig14.eps}
\caption{The overlapping Si~II* 1264.7, 1265.0~\AA\ interstellar-line
profiles toward all four stars.  Where unconfused, the heliocentric radial 
velocities [km~s$^{-1}$] of discrete components are marked, for the
1264.7~\AA\ line at the top of each panel, and for 1265.0~\AA\ at the bottom. 
\label{fig14}}
\end{figure}

\begin{figure}
\centering
\includegraphics[width=5.5in]{fig15.eps}
\caption{The partially overlapping interstellar-line profiles of Si~II
1304, O~I* 1305, and O~I** 1306~\AA\ toward all four stars.  Where
unconfused, the heliocentric radial velocities [km~s$^{-1}$] of discrete 
components are marked, for the O~I** line at the top of each panel, and
for the O~I* at the bottom.  The telluric components of the O~I*, O~I**
are marked with Earth symbols. 
\label{fig15}}
\end{figure}

\begin{figure}
\centering
\includegraphics[width=4in,angle=90]{fig16a.eps}
\end{figure}
\begin{figure}
\centering
\includegraphics[width=4in,angle=90]{fig16b.eps}
\caption{a) Logarithmic column-density ratios of Mg~II/Fe~II versus local 
radial velocity for discrete interstellar components toward all four stars,
which are distinguished by the different symbols given in the key.
Standard values of the ratio from Savage \& Sembach 1996 are marked at the
right, ranging from solar abundances (undepleted) to cool-disk depletions. 
b)~Same for Si~II/Fe~II.
\label{fig16}}
\end{figure}

%\addtocounter{figure}{-1}
%\begin{figure}
%\caption{b) Same for Si~II/Fe~II.
%\label{fig16}}
%\end{figure}

\begin{figure}
\centering
\includegraphics[width=4in,angle=90]{fig17.eps}
\caption{Logarithmic column-density ratios of C~IV/Si~IV versus local
radial velocity for discrete interstellar components toward the four stars,
which are distinguished by the symbols given in the key.  Typical values 
of the ratio for different ionization mechanisms (Franco \& Savage 1982)
are indicated at the right. 
\label{fig17}}
\end{figure}

\begin{landscape}
%\documentclass[10pt,preprint]{aastex}
%\textwidth=9.5in
%\textheight=7in
%\voffset=-.8in
%\hoffset=-.3in
%\pagestyle{empty}
\def\en{\enspace}
%\begin{document}
\begin{deluxetable}{crcclcccc}
\tablewidth{0pt}
\tablecaption{Stellar and Exposure Data}
\tablehead{
\colhead{Star} &\colhead{R.A.\ (2000)} &\colhead{Spectral} &\colhead{$V$} &\colhead{Date} 
&\colhead{Echelle} &\colhead{Central} &\colhead{Exposure} &\colhead{Flux}\\
&\colhead{Dec.\ (2000)} &\colhead{Type} &\colhead{$B-V$} & & &\colhead{Wavelength [\AA]} 
&\colhead{Time [s]} &\colhead{[erg cm$^{-2}$ s$^{-1}$ \AA$^{-1}$]}
}
\startdata               
CPD~$-59^{\circ}$~2603 &10 44 47.42      &O7 V((f))    &8.77 &1997 June 6 &E140H &1416 &1730 &7E$-$12\\
                       &$-$59 43 53.6\en &             &0.14 &            &E230H &2762 &1250 &3E$-$12\\
                       &                 &             &     &1999 Apr 19 &E140H &1234 &5160 &7E$-$12\\
                       &                 &             &     &            &      &1416 &3180 &7E$-$12\\
                       &                 &             &     &            &      &1598 &4800 &7E$-$12\\
                       &                 &             &     &            &E230H &2513 &2820 &3E$-$12\\
                       &                 &             &     &            &      &2762 &2340 &3E$-$12\\
\\
HD~93205               &10 44 33.82      &O3.5 V((f+)) &7.75 &1999 Apr 20 &E140H &1234 &1200 &5E$-$11\\
                       &$-$59 44 15.3\en &+ O8 V       &0.05 &            &      &1416 &\en780 &4E$-$11\\
                       &                 &             &     &            &      &1598 &1380 &4E$-$11\\
                       &                 &             &     &            &E230H &1763 &2220 &3E$-$11\\
                       &                 &             &     &            &      &2513 &\en780 &1E$-$11\\
                       &                 &             &     &            &      &2762 &\en720&1E$-$11\\
\\
HDE~303308             &10 45 05.96      &O4 V((f+))   &8.17 &1998 Mar 19 &E140H &1234 &1680 &2E$-$11\\
                       &$-$59 40 06.4\en &             &0.13 &            &      &1416 &1140 &2E$-$11\\
                       &                 &             &     &            &      &1598 &2460 &2E$-$11\\
                       &                 &             &     &1998 Mar 20 &E230H &1763 &4080 &1E$-$11\\
                       &                 &             &     &            &      &2513 &1080 &6E$-$12\\
                       &                 &             &     &            &      &2762 &1020 &6E$-$12\\
\\
HD~93222               &10 44 36.33      &O7 III((f))  &8.11 &1998 Dec 28 &E140H &1234 &2220 &3E$-$11\\
                       &$-$60 05 28.8\en &             &0.05 &            &      &1416 &1560 &3E$-$11\\
                       &                 &             &     &            &      &1598 &2400 &3E$-$11\\
                       &                 &             &     &            &E230H &1763 &4020 &2E$-$11\\
                       &                 &             &     &            &      &2513 &1380 &9E$-$12\\
                       &                 &             &     &            &      &2762 &1140 &8E$-$12\\
\enddata                                                                                               
\end{deluxetable}
\end{landscape}


%\documentclass[10pt]{paastex}
%\usepackage{myemulateapj5}
%\pagestyle{empty}
%\begin{document}
%\clearpage
\begin{tabular}{llccl}
\multicolumn{5}{c}{Table 2. CPD $-$59\degr 2603}\\
\\
\hline\hline
Ion &\multicolumn{1}{c}{$\lambda$} &v &b &Log N\\
\hline
\multicolumn{5}{c}{$-$233 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & $-$233.00  &     7.48  &    11.08 \\
C II & 1334.532$^{a}$ & $-$232.65  &     3.81  &    12.83 \\
 & 1334.532$^{b}$ &  $-$234.01  &     4.14  &    12.91 \\
Fe II & 1608.451 & $-$232.96  &     1.50  &    12.06: \\
      & 2382.765 & $-$233.63  &     1.57  &    11.52 \\
      & 2586.650 & $-$232.44  &     3.42  &    11.98  \\
      & 2600.173 & $-$233.78  &     2.55  &    11.68 \\
Mg II & 2796.352$^{a}$ & $-$233.45  &     1.89  &    11.49 \\
      & 2796.352$^{b}$ &  $-$233.41  &     3.36  &    11.68 \\
      & 2803.531$^{a}$ & $-$232.07  &     2.92  &    11.69 \\
      & 2803.531$^{b}$ & $-$232.58  &     3.16  &    11.73  \\
O I  & 1302.169 & $-$235.01  &     5.31  &    12.76  \\
Si II & 1304.370 & $-$231.04  &     2.43  &    11.85  \\
      & 1526.707 & $-$232.39  &     1.56  &    11.95 \\
\hline
\multicolumn{5}{c}{$-$216 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & $-$216.09  &     3.96  &    12.29 \\
C II & 1334.532$^{a}$ & $-$214.71  &     5.13  &    14.45: \\
 & 1334.532$^{b}$ &  $-$215.72  &     5.37  &    14.35: \\
Fe II & 1608.451 & $-$216.41  &     3.09  &    13.33  \\
      & 2382.765 & $-$216.26  &     3.60  &    13.45: \\
      & 2586.650 & $-$216.55  &     3.40  &    13.34  \\
      & 2600.173 & $-$216.29  &     4.00  &    13.33 \\
Mg I & 2852.964$^{a}$ & $-$217.12  &     2.74  &    11.61  \\
    & 2852.964$^{b}$ & $-$216.72  &     3.12  &    11.43  \\ 
Mg II & 2796.352$^{a}$ & $-$215.82  &     3.82  &    13.59: \\
      & 2796.352$^{b}$ &  $-$215.45  &     4.35  &    13.28: \\
      & 2803.531$^{a}$ & $-$215.84  &     4.59  &    13.27 \\
      & 2803.531$^{b}$ & $-$215.48  &     4.37  &    13.25  \\
Mn II & 2576.877 & $-$216.71  &     1.50  &    11.28:  \\
O I  & 1302.169 &  $-$216.34  &     4.90  &    14.44  \\
O I** & 1306.029 & $-$215.47  &     4.45  &    12.57  \\
S II & 1253.811 & $-$214.55  &     5.57  &    13.33  \\
     & 1259.519 & $-$216.43  &     3.71  &    13.44  \\
Si II & 1304.370 &  $-$215.80  &     4.82  &    13.55 \\
      & 1526.707 & $-$216.15  &     3.91  &    13.48 \\ 
Si II* & 1264.738 & $-$216.70  &     3.62  &    12.54 \\
      & 1265.002 & $-$216.55  &     2.54  &    12.64  \\
      & 1309.276 & $-$216.85  &     2.92  &    12.18 \\     
\hline
\multicolumn{5}{c}{$-$185 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & $-$185.02  &     1.76  &    11.00 \\
C II & 1334.532$^{a}$ & $-$182.06  &     5.37  &    13.04 \\
    & 1334.532$^{b}$ &  $-$185.30  &     4.08  &    13.09 \\
Fe II & 1608.451 &  $-$187.12  &     1.69  &    12.34 \\
      & 2382.765 & $-$185.64  &     2.18  &    12.06 \\
      & 2586.650 & $-$185.33  &     4.05  &    12.20  \\
      & 2600.173 &  $-$185.39  &     2.45  &    12.09 \\
Mg I & 2852.964$^{b}$ & $-$186.03  &     1.50  &    10.30: \\
Mg II & 2796.352$^{a}$ & $-$183.18  &     3.26  &    11.54 \\
      & 2796.352$^{b}$ & $-$185.11  &     3.40  &    11.88 \\
      & 2803.531$^{a}$ & $-$182.43  &     3.44  &    11.66 \\
      & 2803.531$^{b}$ & $-$184.51  &     3.05  &    11.81  \\
O I  & 1302.169 & $-$185.64  &     3.90  &    13.03  \\
S II & 1253.811 & $-$181.30  &     1.50  &    13.24  \\
\end{tabular}
%
\hspace{.4in}\hbox{
\begin{tabular}{llcrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &v &\multicolumn{1}{c}{b} &Log N\\
\hline
Si II & 1304.370 &  $-$185.05  &     4.61  &    12.51 \\
      & 1526.707 & $-$184.12  &     5.39  &    12.56 \\ 
\hline
\multicolumn{5}{c}{$-$166 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & $-$165.54  &     4.47  &    12.33 \\
C II & 1334.532$^{a}$ & $-$165.27  &     5.59  &    14.32: \\
     & 1334.532$^{b}$ &  $-$166.30  &     6.32  &    14.32: \\
Fe II & 1608.451 & $-$166.26  &     4.27  &    13.18\\
      & 2382.765 & $-$166.74  &     4.35  &    13.07 \\
      & 2586.650 & $-$165.87  &     3.57  &    13.07  \\
      & 2600.173 &  $-$166.35  &     4.26  &    13.08 \\
Mg I & 2852.964$^{a}$ & $-$165.90  &     4.67  &    11.11 \\
     & 2852.964$^{b}$ &  $-$165.41  &     4.00  &    11.11  \\ 
Mg II & 2796.352$^{a}$ & $-$165.77  &     4.81  &    12.97 \\
      & 2796.352$^{b}$ & $-$166.02  &     5.33  &    12.97 \\
      & 2803.531$^{a}$ & $-$165.29  &     4.65  &    13.00 \\
      & 2803.531$^{b}$ & $-$165.18  &     5.09  &    12.98  \\
O I  & 1302.169 &  $-$165.84  &     4.70  &    13.81  \\
S II & 1250.584 & $-$166.00  &     6.04  &    13.65  \\
     & 1253.811 & $-$166.00  &     7.00  &    13.54 \\
     & 1259.519 &  $-$165.82  &     4.56  &    13.19  \\
Si II & 1304.370 & $-$165.71  &     4.56  &    13.42 \\
      & 1526.707 & $-$165.74  &     4.93  &    13.42 \\ 
Si II* & 1264.738 & $-$165.40  &     3.95  &    11.52 \\
%       &     &     &     &     \\
C IV & 1548.195 &   $-$170.43  &    12.00  &    12.66  \\
\hline
\multicolumn{5}{c}{$-$153 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & $-$153.10  &     5.15  &    11.80 \\
C II & 1334.532$^{a}$ & $-$153.55  &     7.43  &    13.99 \\
    & 1334.532$^{b}$ &  $-$153.27  &     6.87  &    13.92 \\
Fe II & 1608.451 & $-$153.25  &     2.15  &    12.44 \\
      & 2382.765 & $-$154.11  &     3.43  &    12.38 \\
      & 2586.650 & $-$153.96  &     3.58  &    12.45  \\
      & 2600.173 &  $-$153.92  &     3.49  &    12.43 \\
Mg I & 2852.964$^{a}$ &  $-$151.33  &     1.50  &    10.30: \\
     & 2852.964$^{b}$ &  $-$152.72  &     1.97  &    10.48:  \\ 
Mg II & 2796.352$^{a}$ & $-$153.76  &     4.62  &    12.41 \\
      & 2796.352$^{b}$ & $-$153.12  &     4.41  &    12.37 \\
      & 2803.531$^{a}$ &  $-$153.54  &     4.74  &    12.42 \\
      & 2803.531$^{b}$ &  $-$152.55  &     3.67  &    12.37  \\
O I  & 1302.169 & $-$153.59  &     3.87  &    13.29  \\
Si II & 1304.370 & $-$152.38  &     4.14  &    12.73 \\
      & 1526.707 & $-$152.91  &     3.94  &    12.80 \\ 
%       &     &     &     &     \\
C IV & 1548.195 &  $-$149.19  &    12.00  &    12.94 \\
    &  1550.770 &  $-$155.46  &    12.00  &    12.72 \\
Si IV & 1393.755$^{a}$ & $-$156.70  &    12.00  &    12.27 \\
      & 1393.755$^{b}$ &  $-$158.72  &     9.31  &    12.15 \\
     & 1402.770$^{a}$ & $-$160.49  &     6.41  &    12.23 \\	
     & 1402.770$^{b}$ & $-$158.43  &    12.00  &    12.38 \\
\hline
\multicolumn{5}{c}{$-$137 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & $-$136.44  &     7.34  &    11.51 \\
C II & 1334.532$^{a}$ & $-$134.49  &     9.00  &    13.81 \\
     & 1334.532$^{b}$ & $-$135.92  &     8.50  &    13.78 \\
Fe II  & 2382.765 & $-$138.29  &     2.66  &    11.76 \\
      & 2586.650 & $-$136.79  &     2.92  &    11.83 \\
      & 2600.173 &  $-$138.39  &     5.24  &    11.94 \\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Mg II & 2796.352$^{a}$ & $-$136.51  &     7.10  &    12.07 \\
      & 2796.352$^{b}$ & $-$136.65  &     7.19  &    12.13 \\
      & 2803.531$^{a}$ & $-$136.36  &     7.01  &    12.18 \\
      & 2803.531$^{b}$ & $-$136.87  &     8.00  &    12.23  \\
Si II & 1304.370 & $-$137.00  &     2.32  &    11.20: \\
      & 1526.707 & $-$139.10  &     6.46  &    12.44 \\ 
\hline
\multicolumn{5}{c}{$-$120 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 &  $-$119.85  &     4.81  &    11.68 \\
C II & 1334.532$^{a}$ & $-$117.65  &     6.93  &    13.99: \\
     & 1334.532$^{b}$ &  $-$120.31  &     6.46  &    13.90: \\
C II* & 1335.708$^{a}$ & $-$119.54  &     6.31  &    13.54 \\
     & 1335.708$^{b}$ & $-$121.09  &     4.60  &    13.41 \\
 Fe II & 2382.765 & $-$120.86  &     3.67  &    12.40 \\
      & 2586.650 & $-$120.83  &     4.36  &    12.46 \\
      & 2600.173 &  $-$120.53  &     4.08  &    12.48 \\
Mg I & 2852.964$^{a}$ &  $-$119.47  &     1.87  &    10.48: \\
     & 2852.964$^{b}$ &  $-$120.08  &     4.96  &    10.78  \\ 
Mg II & 2796.352$^{a}$ & $-$119.97  &     4.34  &    12.47 \\
      & 2796.352$^{b}$ & $-$120.17  &     4.07  &    12.52 \\
      & 2803.531$^{a}$ &  $-$119.50  &     4.70  &    12.52 \\
      & 2803.531$^{b}$ &  $-$119.57  &     4.56  &    12.58  \\
O I  & 1302.169 & $-$120.42  &     4.30  &    13.65 \\
Si II & 1304.370 &  $-$119.24  &     4.25  &    12.59 \\
      & 1526.707 & $-$120.05  &     4.66  &    12.80 \\ 
Si II* & 1264.738 & $-$121.72  &     2.48  &    11.26  \\
%       &     &     &     &     \\
C IV & 1548.195 & $-$128.38  &    12.00  &    13.06 \\
    &  1550.770  & $-$125.89  &    12.00  &    13.03  \\
Si IV & 1402.770$^{a}$ &  $-$127.31  &    12.00  &    12.52 \\	
     & 1402.770$^{b}$ & $-$127.79  &    12.00  &    12.66 \\			
\hline
\multicolumn{5}{c}{$-$101 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & $-$98.65  &     9.80  &    12.45 \\
C II* & 1335.708$^{a}$ & $-$99.96  &     9.41  &    13.83: \\
      & 1335.708$^{b}$ & $-$99.77  &    10.00  &    13.84: \\
Fe II & 1608.451 & $-$101.75  &     3.01  &    12.71  \\
       & 1611.201 & $-$102.62  &     2.37  &    13.89  \\
      & 2382.765 & $-$102.38  &     6.78  &    12.94 \\
      & 2586.650 & $-$101.98  &     6.91  &    12.96 \\
      & 2600.173 &  $-$102.28  &     6.64  &    12.93 \\
Mg I & 2852.964$^{a}$ &  $-$100.98  &     8.06  &    11.11 \\
     & 2852.964$^{b}$ &   $-$97.24  &     7.00  &    11.04 \\ 
Mg II & 2796.352$^{a}$ & $-$97.58  &     8.72  &    13.43: \\
      & 2796.352$^{b}$ & $-$97.96  &     9.34  &    13.35: \\
      & 2803.531$^{a}$ &  $-$98.57  &     8.06  &    13.28 \\
      & 2803.531$^{b}$ &  $-$98.08  &     8.52  &    13.35  \\
S II & 1253.811 & $-$101.00  &     8.00  &    13.37  \\
     & 1259.519 & $-$100.00  &     7.00  &    13.27  \\
Si II & 1304.370 &  $-$99.03  &     7.46  &    13.62 \\
      & 1526.707 & $-$99.50  &     7.33  &    13.60 \\ 
%       &     &     &     &     \\
C IV & 1548.195 & $-$113.00  &    11.32  &    13.02 \\
     & 1548.195 & $-$97.62  &     7.09  &    12.94 \\
    &  1550.770  & $-$96.39  &    12.00  &    13.15  \\
Si IV & 1402.770$^{a}$ & $-$99.03  &     9.36  &    12.61 \\	
     & 1402.770$^{b}$ & $-$101.78  &     9.00  &    12.73 \\	
\end{tabular}
%
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\multicolumn{5}{c}{$-$77 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 &  $-$77.69  &    10.00  &    12.67 \\
Fe II & 1608.451 & $-$76.10  &     8.79  &    12.93 \\
      & 2382.765 & $-$77.78  &    10.00  &    13.13 \\
      & 2586.650 & $-$80.48  &    10.00  &    13.02 \\
      & 2600.173 &  $-$78.76  &    10.00  &    13.08 \\
Mg I & 2852.964$^{a}$ &  $-$77.11  &    10.00  &    11.82 \\
     & 2852.964$^{b}$ &  $-$77.67  &    10.00  &    11.72  \\ 
Mg II & 2796.352$^{a}$ & $-$74.86  &    10.00  &    13.63: \\
      & 2796.352$^{b}$ & $-$77.54  &    10.00  &    13.41: \\
      & 2803.531$^{a}$ &  $-$75.77  &    10.00  &    13.79: \\
      & 2803.531$^{b}$ &  $-$75.88  &     8.38  &    13.97: \\
Mn II & 2594.499 & $-$77.00  &     6.00  &    11.62 \\
P II & 1532.533 & $-$79.12  &     1.50  &    12.78: \\
S II & 1250.584 &  $-$78.62  &     6.00  &    13.81  \\
   & 1253.811 & $-$77.00  &     9.00  &    14.03 \\
   & 1259.519  & $-$75.94  &     9.00  &    13.97 \\
Si II & 1304.370 & $-$76.06  &    10.00  &    13.95 \\
      & 1526.707 & $-$76.21  &    10.00  &    13.97 \\
%       &     &     &     &     \\
C IV & 1548.195 & $-$83.56  &    12.00  &    13.12 \\
Si IV & 1402.770$^{a}$ & $-$85.67  &     7.64  &    12.60 \\	
     & 1402.770$^{b}$ & $-$88.34  &     7.46  &    12.71 \\
\hline
\multicolumn{5}{c}{$-$63 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 &   $-$63.85  &     9.80  &    12.26 \\
Fe II & 1608.451 & $-$64.20  &     3.05  &    12.56 \\
      & 2382.765 & $-$63.82  &     4.75  &    12.57 \\
      & 2586.650 & $-$65.85  &     8.50  &    12.91 \\
      & 2600.173 & $-$64.65  &     7.00  &    12.77 \\
Mg I & 2852.964$^{a}$ &  $-$63.00  &     6.71  &    10.78 \\
     & 2852.964$^{b}$ &  $-$63.00  &     7.49  &    11.18  \\ 
Mg II & 2796.352$^{a}$ & $-$63.00  &     9.00  &    12.81: \\
      & 2796.352$^{b}$ & $-$63.00  &     5.04  &    12.92: \\
      & 2803.531$^{a}$ & $-$60.06  &     2.01  &    12.31: \\
      & 2803.531$^{b}$ &  $-$61.60  &     4.27  &    12.66: \\
Mn II & 2594.499 & $-$63.12  &     4.29  &    11.34: \\
O I] & 1355.598$^{a}$ &  $-$63.90  &     5.16  &    17.28  \\
S II & 1250.584 &   $-$63.00  &     7.85  &    13.53  \\
   & 1253.811 & $-$63.00  &     7.00  &    13.68 \\
   & 1259.519  & $-$63.00  &     6.00  &    13.32 \\
Si II & 1304.370 & $-$64.00  &     7.14  &    13.23 \\
      & 1526.707 & $-$63.92  &     7.06  &    13.28 \\ 
%       &     &     &     &     \\
C IV & 1548.195 & $-$65.00  &    12.00  &    12.85 \\
    &  1550.770  &  $-$65.17  &     9.83  &    12.54 \\
Si IV & 1393.755$^{a}$ &  $-$70.99  &    11.60  &    12.60 \\
      & 1393.755$^{b}$ & $-$70.22  &    12.00  &    12.44 \\
     & 1402.770$^{a}$ & $-$70.99  &     9.54  &    12.30 \\	
     & 1402.770$^{b}$ &  $-$71.04  &    12.00  &    12.70 \\			
\hline
\multicolumn{5}{c}{$-$38 km s$^{-1}$ Component}  \\
\hline
Cl I & 1347.240$^{a}$ & $-$36.24  &     2.77  &    12.00  \\
Cu II & 1358.773$^{a}$ & $-$38.21  &     3.86  &    11.89  \\
      & 1358.773$^{b}$ &  $-$35.92  &     4.47  &    11.88  \\
Fe I & 2484.021 & $-$37.74  &     5.01  &    11.46 \\
\\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Fe II & 1608.451 &  $-$38.80  &     3.60  &    15.64: \\ 
      & 1611.201 & $-$38.65  &     5.67  &    14.90 \\
     & 2586.650 & $-$37.94  &     3.87  &    15.90:  \\
Ga II & 1414.402$^{a}$ &  $-$36.33  &     2.72  &    10.60 \\
      & 1414.402$^{b}$ &   $-$40.08  &     1.98  &    10.78 \\
Ge II & 1237.059 & $-$36.07  &     5.72  &    11.41  \\
Mg I & 1683.412 & $-$41.39  &     1.50  &    13.54 \\
    & 2852.964$^{a}$ & $-$37.41  &     5.61  &    12.89:  \\
    & 2852.964$^{b}$ &  $-$37.15  &     5.32  &    13.11:  \\
Mg II & 1239.925 & $-$36.54  &     5.40  &    15.49  \\
      & 1240.395 & $-$37.13  &     4.98  &    15.46  \\
Mn II & 2576.877 & $-$37.57  &     6.27  &    13.03  \\
      & 2594.499 & $-$37.74  &     6.26  &    13.02  \\
      & 2606.462 &  $-$37.83  &     6.36  &    13.01 \\
Ni II & 1317.217$^{a}$ & $-$38.10  &     5.05  &    13.51 \\
      & 1317.217$^{b}$ & $-$38.21  &     5.16  &    13.48  \\
       & 1370.132$^{a}$ & $-$37.26  &     5.28  &    13.51 \\
       & 1370.132$^{b}$ & $-$37.50  &     4.70  &    13.49  \\
      & 1454.842$^{a}$  & $-$36.78  &     3.83  &    13.20  \\
       & 1454.842$^{b}$  &  $-$38.01  &     4.03  &    13.18  \\
O I* & 1304.858 &  $-$36.63  &     4.32  &    13.68  \\
O I** & 1306.029 & $-$37.26  &     4.72  &    13.72  \\
S II & 1250.584 & $-$36.75  &     5.68  &    15.63: \\
Si II* & 1264.738 & $-$33.00  &     6.80  &    14.71: \\
       & 1265.002 & $-$33.94  &     6.89  &    14.34:  \\
       & 1309.276 & $-$33.96  &     6.57  &    14.12 \\
       & 1533.431 & $-$34.00  &     7.11  &    14.29:  \\
%       &     &     &     &     \\
C IV & 1548.195 & $-$43.38  &     5.88  &    14.05: \\
    &  1550.770  &  $-$43.92  &     5.06  &    14.08 \\
Si IV & 1393.755$^{a}$ & $-$43.85  &     4.77  &    14.64: \\
      & 1393.755$^{b}$ & $-$43.54  &     5.28  &    14.38: \\
     & 1402.770$^{a}$ & $-$46.24  &     4.05  &    14.37: \\	
     & 1402.770$^{b}$ & $-$44.60  &     5.24  &    14.38: \\	
\hline
\multicolumn{5}{c}{$-$28 km s$^{-1}$ Component}  \\
\hline
Cl I & 1347.240$^{a}$ & $-$27.71  &     3.61  &    12.01 \\
Cu II & 1358.773$^{a}$ & $-$28.00  &     4.00  &    11.89  \\
Fe II & 1608.451 &  $-$28.00  &     2.46  &    14.10: \\ 
      & 1611.201 & $-$28.26  &     1.50  &    14.05 \\
     & 2586.650 & $-$28.00  &     2.58  &    14.79:  \\
Ga II & 1414.402$^{a}$ &  $-$27.84  &     1.50  &    10.70: \\
Mg I  & 2852.964$^{a}$ & $-$28.00  &     1.50  &    13.22: \\
    & 2852.964$^{b}$ &  $-$28.00  &     2.50  &    11.99:  \\
Mg II & 1239.925 &  $-$28.01  &     2.37  &    14.90 \\
      & 1240.395 & $-$27.44  &     1.50  &    14.79 \\
Mn II & 2576.877 & $-$27.78  &     1.92  &    12.14  \\
      & 2594.499 & $-$28.09  &     2.19  &    12.21 \\
      & 2606.462 &  $-$28.81  &     1.53  &    11.97 \\
Ni II & 1317.217$^{a}$ & $-$26.97  &     2.73  &    12.68 \\
      & 1317.217$^{b}$ & $-$28.07  &     1.50  &    12.27 \\
       & 1370.132$^{a}$ & $-$26.31  &     1.68  &    12.57 \\
       & 1370.132$^{b}$ & $-$27.42  &     2.66  &    12.66  \\
      & 1454.842$^{a}$  & $-$28.22  &     3.95  &    12.41 \\
       & 1454.842$^{b}$  &  $-$26.42  &     1.50  &    12.23: \\
O I* & 1304.858 &  $-$27.96  &     2.95  &    13.24  \\
O I** & 1306.029 & $-$28.96  &     2.33  &    13.10  \\
S II & 1250.584 & $-$28.00  &     1.70  &    15.20: \\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
%       &     &     &     &     \\
C IV & 1548.195 & $-$29.67  &     5.74  &    13.82: \\
    &  1550.770  & $-$30.92  &     6.45  &    14.01  \\
Si IV & 1393.755$^{a}$ & $-$28.62  &     3.90  &    14.26: \\
      & 1393.755$^{b}$ & $-$29.88  &     4.49  &    14.23: \\
     & 1402.770$^{a}$ & $-$32.70  &     6.46  &    14.26: \\	
     & 1402.770$^{b}$ &  $-$30.37  &     3.88  &    14.57: \\	
\hline
\multicolumn{5}{c}{$-$19 km s$^{-1}$ Component}  \\
\hline
Cu II & 1358.773$^{a}$ & $-$18.56  &     2.64  &    11.89  \\
    & 1358.773$^{b}$ & $-$19.45  &     2.00  &    11.89  \\
Fe II & 1608.451 &  $-$19.00  &     4.11  &    14.19: \\ 
      & 1611.201 & $-$18.85  &     3.55  &    14.81 \\
Ga II & 1414.402$^{a}$ &   $-$19.34  &     2.09  &    11.08 \\
    & 1414.402$^{b}$ & $-$19.08  &     1.50  &    11.04  \\
Ge II & 1237.059 & $-$19.21  &     2.08  &    11.76  \\
Mg I  & 2852.964$^{a}$ & $-$19.00  &     5.02  &    12.48: \\
    & 2852.964$^{b}$ & $-$19.00  &     6.87  &    12.58: \\
Mg II & 1239.925 &  $-$18.25  &     4.27  &    15.61 \\
      & 1240.395 & $-$18.33  &     3.29  &    15.56 \\
Mn II & 2576.877 & $-$17.82  &     4.19  &    13.52 \\
      & 2594.499 & $-$17.93  &     4.26  &    13.47 \\
      & 2606.462 &  $-$18.91  &     4.53  &    13.43 \\
Ni II & 1317.217$^{a}$ & $-$16.56  &     4.97  &    13.09 \\
      & 1317.217$^{b}$ & $-$17.02  &     5.94  &    13.07 \\
       & 1370.132$^{a}$ & $-$16.37  &     4.86  &    13.07 \\
       & 1370.132$^{b}$ & $-$16.82  &     4.06  &    13.00  \\
      & 1454.842$^{a}$  & $-$16.70  &     4.12  &    12.75 \\
       & 1454.842$^{b}$  &   $-$16.72  &     3.47  &    12.57 \\
O I] & 1355.598$^{a}$ & $-$19.34  &     2.11  &    17.58  \\
    & 1355.598$^{b}$ & $-$19.03  &     2.58  &    17.50  \\
O I** & 1306.029 & $-$15.61  &     8.80  &    13.71  \\
P II & 1532.533 & $-$19.09  &     3.51  &    13.96  \\
S II & 1250.584 & $-$19.00  &     5.70  &    15.46: \\
Si II* & 1264.738 &  $-$18.83  &     7.31  &    13.50:  \\
        & 1265.002  & $-$17.32  &     6.48  &    13.24  \\
	& 1309.276 & $-$17.21  &     5.84  &    12.95  \\
	& 1533.431 &  $-$17.00  &     6.14  &    13.28  \\
%       &     &     &     &     \\
C IV & 1548.195 & $-$19.00  &     8.00  &    13.18 \\
    &  1550.770  &  $-$19.00  &    10.00  &    13.08 \\
Si IV & 1393.755$^{a}$ & $-$19.00  &     5.00  &    12.30 \\
      & 1393.755$^{b}$ & $-$19.00  &     9.00  &    12.38 \\
     & 1402.770$^{a}$ & $-$19.00  &     8.00  &    12.17 \\	
     & 1402.770$^{b}$ & $-$19.00  &     3.20  &    12.23 \\	
\hline
\multicolumn{5}{c}{$-$3 km s$^{-1}$ Component}\\
\hline
Cl I & 1347.240$^{a}$ & $-$5.03  &     4.61  &    12.67  \\
     &  1347.240$^{b}$ & $-$4.85  &     4.76  &    12.72  \\
Cu II & 1358.773$^{a}$ & $-$4.84  &     4.43  &    11.99  \\
    & 1358.773$^{b}$ & $-$3.13  &     7.00  &    12.14  \\
Fe I & 2484.021 & $-$2.68  &     2.12  &    11.08  \\
Fe II & 1608.451 & $-$2.00  &     7.00  &    15.48: \\ 
      & 1611.201 & $-$3.51  &     5.92  &    15.02 \\
Ga II & 1414.402$^{b}$ & $-$2.32  &     8.09  &    11.26 \\
Ge II & 1237.059 & $-$4.78  &     7.00  &    11.63  \\
Mg I  & 2852.964$^{a}$ & $-$2.00  &     8.00  &    13.25: \\
    & 2852.964$^{b}$ & $-$2.00  &     8.00  &    13.08: \\
Mg II & 1239.925 &   $-$2.86  &     5.00  &    15.68 \\
      & 1240.395 & $-$2.88  &     5.06  &    15.64 \\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Mn II & 2576.877 & $-$3.75  &     5.00  &    13.28 \\
      & 2594.499 & $-$3.73  &     5.00  &    13.28 \\
      & 2606.462 &  $-$3.76  &     6.00  &    13.32 \\
Ni II & 1317.217$^{a}$ & $-$3.60  &     4.86  &    13.54 \\
      & 1317.217$^{b}$ & $-$2.86  &     5.39  &    13.53 \\
       & 1370.132$^{a}$ & $-$2.47  &     4.97  &    13.56 \\
       & 1370.132$^{b}$ & $-$2.30  &     6.03  &    13.64  \\
      & 1454.842$^{a}$  & $-$3.08  &     4.30  &    13.23 \\
       & 1454.842$^{b}$  &   $-$2.09  &     6.10  &    13.34 \\
O I] & 1355.598$^{a}$ & $-$2.84  &     7.00  &    17.48  \\
    & 1355.598$^{b}$ & $-$3.44  &     7.00  &    17.36  \\
P II & 1532.533 &  $-$2.75  &     7.00  &    14.00  \\
S II & 1250.584 &  $-$2.00  &     6.00  &    16.82: \\
Si II* & 1264.738 &  $-$2.32  &     1.97  &    12.41  \\
        & 1265.002  & $-$1.33  &     2.69  &    12.44  \\
	& 1309.276 & $-$2.82  &     2.21  &    12.14  \\
	& 1533.431 &  $-$2.55  &     2.27  &    12.51  \\
%       &     &     &     &     \\
C IV & 1548.195 & $-$5.72  &     8.00  &    12.98 \\
    &  1550.770  &  $-$5.77  &     8.00  &    12.76 \\
Si IV & 1393.755$^{a}$ & $-$7.06  &     7.48  &    12.24 \\
      & 1393.755$^{b}$ & $-$4.36  &     3.65  &    11.97 \\
     & 1402.770$^{a}$ &  $-$5.12  &     8.16  &    12.30 \\	
     & 1402.770$^{b}$ &  $-$6.68  &     7.83  &    12.42 \\	
\hline
\multicolumn{5}{c}{8 km s$^{-1}$ Component}\\
\hline
Cl I & 1347.240$^{a}$ & 6.91  &     3.56  &    13.89  \\
     &  1347.240$^{b}$ & 6.90  &     3.09  &    14.15  \\
Cu II & 1358.773$^{a}$ & 7.43  &     4.57  &    12.44  \\
    & 1358.773$^{b}$ & 8.15  &     2.81  &    12.24 \\
Fe I & 2484.021 & 7.52  &     3.46  &    11.79  \\
Fe II & 1608.451 & 8.00  &     7.40  &    15.22: \\ 
      & 1611.201 & 7.63  &     3.59  &    15.00 \\
Ga II & 1414.402$^{a}$ & 7.68  &     2.06  &    11.38 \\
      & 1414.402$^{b}$ & 8.31  &     2.03  &    11.51  \\
Ge II & 1237.059 & 8.09  &     3.07  &    12.23  \\
Mg I & 1683.412 & 8.02  &     1.96  &    14.18 \\
     & 2852.964$^{a}$ &  8.00  &     7.00  &    12.94: \\
    & 2852.964$^{b}$ & 8.00  &     7.00  &    13.10: \\
Mg II & 1239.925 &   8.14  &     3.82  &    15.99 \\
      & 1240.395 &  8.15  &     3.68  &    16.03 \\
Mn II & 2576.877 & 6.98  &     4.00  &    13.82: \\
      & 2594.499 & 7.12  &     3.71  &    13.88 \\
      & 2606.462 &   7.05  &     4.06  &    13.68 \\
Ni II & 1317.217$^{a}$ & 7.58  &     4.67  &    13.68 \\
      & 1317.217$^{b}$ &  7.74  &     4.60  &    13.60 \\
       & 1370.132$^{a}$ &  8.26  &     4.87  &    13.67 \\
       & 1370.132$^{b}$ & 8.31  &     4.35  &    13.61  \\
      & 1454.842$^{a}$  & 8.12  &     4.94  &    13.42 \\
       & 1454.842$^{b}$  &    8.05  &     3.76  &    13.26 \\
O I] & 1355.598$^{a}$ & 7.50  &     2.93  &    17.72  \\
    & 1355.598$^{b}$ & 8.29  &     2.05  &    17.70 \\
O I** & 1306.029 & 8.73  &     4.50  &    12.62  \\
P II & 1532.533 & 7.68  &     2.73  &    14.30 \\
S I & 1401.514$^{a}$  &  8.23  &     1.52  &    13.52  \\
   & 1401.514$^{b}$  & 7.87  &     1.95  &    13.34  \\
   & 1425.030$^{a}$  & 7.79  &     2.34  &    13.18  \\
    & 1425.030$^{b}$  &  7.16  &     2.20  &    13.24  \\
\end{tabular}
%
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
    & 1425.188$^{a}$  & 8.44  &     1.50  &    13.43  \\
    & 1425.188$^{b}$  &  7.88  &     1.57  &    13.31  \\
S II & 1250.584 &  8.00  &     8.88  &    15.66: \\
Si I & 2515.073 & 7.85  &     1.79  &    12.27  \\
Si II* & 1264.738 & 7.23  &     1.50  &    11.20 \\
	& 1533.431 &  7.99  &     1.50  &    11.85 \\
%       &     &     &     &     \\
C IV & 1548.195 &  5.00  &     8.00  &    12.95 \\
    &  1550.770  &  4.04  &     5.66  &    12.72 \\
Si IV & 1393.755$^{a}$ & 5.70  &     7.39  &    12.45 \\
      & 1393.755$^{b}$ & 5.76  &     5.34  &    12.34 \\
     & 1402.770$^{a}$ &   6.51  &     6.62  &    12.44 \\	
     & 1402.770$^{b}$ & 5.26  &     6.30  &    12.38 \\	
\hline
\multicolumn{5}{c}{17 km s$^{-1}$ Component}\\
\hline
Fe II  & 1611.201 & 15.67  &     1.50  &    13.88 \\
Mn II & 2576.877 & 16.69  &     2.50  &    11.96 \\
      & 2594.499 & 17.27  &     2.50  &    11.97 \\
      & 2606.462 &  17.53  &     2.66  &    11.94 \\
Ni II & 1317.217$^{a}$ & 18.06  &     1.50  &    12.55 \\
      & 1317.217$^{b}$ &  16.95  &     1.50  &    12.41 \\
       & 1370.132$^{a}$ & 18.51  &     1.54  &    12.40 \\
       & 1370.132$^{b}$ & 18.12  &     2.55  &    12.58  \\
      & 1454.842$^{a}$  & 18.64  &     1.50  &    12.17: \\
%       &     &     &     &     \\
C IV & 1548.195 & 16.55  &     6.97  &    12.70 \\
    &  1550.770  &  16.11  &     7.74  &    12.70 \\
Si IV & 1393.755$^{a}$ & 16.56  &     7.33  &    12.16 \\
      & 1393.755$^{b}$ & 16.17  &     7.47  &    12.13 \\
     & 1402.770$^{a}$ & 19.07  &     6.92  &    12.18 \\	
     & 1402.770$^{b}$ & 16.40  &     5.08  &    12.10 \\	
\hline
\multicolumn{5}{c}{26 km s$^{-1}$ Component}\\
\hline
Cl I & 1347.240$^{b}$ & 27.81  &     1.50  &    11.68:  \\
Fe I & 2484.021 & 25.68  &     1.50  &    11.23 \\
Fe II & 1608.451 & 26.17  &     2.03  &    14.10 \\ 
      & 1611.201 & 25.51  &     1.50  &    14.01 \\
      & 2586.650 & 26.05  &     2.09  &    14.41  \\
Mg I & 2852.964$^{a}$ &  24.83  &     4.69  &    12.01 \\
    & 2852.964$^{b}$ & 25.13  &     4.08  &    12.03 \\
Mg II & 1239.925 & 26.18  &     1.50  &    14.29 \\
      & 1240.395 &   21.02  &     5.57  &    14.94 \\
Mn II & 2576.877 &  24.10  &     5.16  &    12.09 \\
      & 2594.499 & 25.11  &     4.86  &    12.13 \\
      & 2606.462 &   25.01  &     3.58  &    11.86 \\
Ni II & 1317.217$^{a}$ & 25.49  &     2.97  &    12.52 \\
      & 1317.217$^{b}$ & 25.02  &     3.66  &    12.68 \\
       & 1370.132$^{a}$ & 26.07  &     3.69  &    12.66 \\
       & 1370.132$^{b}$ & 26.16  &     2.09  &    12.54 \\
      & 1454.842$^{a}$  &  27.50  &     1.50  &    12.20: \\
P II & 1532.533 & 25.13  &     1.50  &    13.00: \\
S II & 1250.584 &  26.00  &     4.45  &    14.05 \\
    & 1253.811 & 26.00  &     6.21  &    14.20  \\
\hline
\multicolumn{5}{c}{38 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & 38.33  &     3.19  &    11.28 \\
Fe II & 2382.765 & 37.34  &     2.44  &    12.25  \\
      & 2586.650 & 37.73  &     2.11  &    12.29  \\
      & 2600.173 & 37.56  &     3.02  &    12.30  \\
Mg I  & 2852.964$^{a}$ & 37.66  &     1.50  &    10.48: \\
\\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Mg II   & 1240.395 &   36.29  &     1.50  &    14.50: \\
      & 2796.352$^{a}$  & 38.91  &     2.90  &    12.20  \\
       & 2796.352$^{b}$  & 37.69  &     3.59  &    12.38  \\
       & 2803.531$^{a}$   & 39.30  &     2.14  &    12.19  \\
       & 2803.531$^{b}$   & 37.41  &     4.14  &    12.40  \\
S II & 1253.811 & 43.93  &     3.69  &    13.23 \\
Si II & 1304.370 & 39.09  &     3.27  &    12.69 \\
     & 1526.707 &  38.06  &     4.19  &    12.79  \\
%       &     &     &     &     \\
C IV & 1548.195 & 33.20  &    12.00  &    12.52  \\     
\hline
\multicolumn{5}{c}{61 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & 62.80  &     3.10  &    10.30: \\
C II* & 1335.708$^{a}$  & 62.76  &     2.74  &    13.00  \\
      & 1335.708$^{b}$  & 61.67  &     3.14  &    13.35  \\
Fe II & 2382.765 & 61.58  &     2.07  &    11.20  \\
      & 2586.650 & 62.52  &     1.50  &    11.81: \\
      & 2600.173 & 60.48  &     2.72  &    11.45 \\
Mg II  & 2796.352$^{a}$  & 61.91  &     2.51  &    11.95 \\
       & 2796.352$^{b}$  & 61.81  &     2.72  &    11.97 \\
       & 2803.531$^{a}$   & 62.49  &     2.51  &    12.03  \\
       & 2803.531$^{b}$   & 61.67  &     2.21  &    11.93  \\
O I & 1302.169 & 61.42  &     3.25  &    13.57  \\
Si II  & 1526.707 &  59.75  &     5.54  &    12.31  \\    
\hline
\multicolumn{5}{c}{69/72 km s$^{-1}$ Component}\\
\hline
C II* & 1335.708$^{a}$  &  67.24  &     7.17  &    13.31 \\
      & 1335.708$^{b}$  & 71.46  &     3.09  &    12.06 \\
Fe II & 2382.765 & 72.23  &     2.00  &    11.08  \\
      & 2600.173 & 72.07  &     2.72  &    11.11: \\
Mg II  & 2796.352$^{a}$  & 69.06  &     3.26  &    11.94 \\
       & 2796.352$^{b}$  & 71.62  &     3.41  &    11.32 \\
       & 2803.531$^{a}$   & 69.04  &     1.90  &    11.90  \\
       & 2803.531$^{b}$   & 73.09  &     2.45  &    11.20 \\
%       &     &     &     &     \\
C IV & 1548.195 & 66.28  &    12.00  &    12.45  \\
\hline
\multicolumn{5}{c}{98 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & 98.16  &     3.39  &    12.21 \\
C II* & 1335.663$^{a}$  &  99.45  &     3.45  &    14.23  \\
      & 1335.663$^{b}$  &  97.88  &     3.90  &    14.27 \\
      & 1335.708$^{a}$  &  99.45  &     3.45  &    14.23  \\
      & 1335.708$^{b}$  &  97.88  &     3.90  &    14.27 \\
Fe II & 1608.451 & 97.83  &     3.39  &    13.34  \\
      & 2382.765 & 97.74  &     1.98  &    14.39: \\
      & 2586.650 & 98.10  &     3.51  &    13.34 \\
      & 2600.173 & 98.14  &     1.90  &    14.57: \\
Mg I & 2852.964$^{a}$  & 99.71  &     3.13  &    11.20  \\
     & 2852.964$^{b}$  & 98.51  &     4.09  &    11.38  \\
Mg II  & 2796.352$^{a}$  & 98.77  &     2.36  &    13.53: \\
       & 2796.352$^{b}$  & 98.30  &     2.54  &    14.13: \\
       & 2803.531$^{a}$   & 98.44  &     2.79  &    13.29  \\
       & 2803.531$^{b}$   & 97.97  &     2.44  &    14.14  \\
Mn II & 2576.877 & 97.54  &     2.95  &    11.26  \\
    & 2594.499  & 97.99  &     4.99  &    11.43  \\
    & 2606.462 & 95.40  &     2.11  &    11.41  \\
Ni II & 1317.217$^{a}$  & 93.96  &     7.62  &    12.93  \\
     & 1317.217$^{b}$  & 101.33  &     4.18  &    12.37  \\
     & 1370.132$^{a}$ &  97.65  &     1.56  &    12.10:  \\
     & 1454.842$^{b}$ & 94.71  &     5.07  &    12.45  \\
O I & 1302.169 &  97.94  &     3.21  &    14.80:  \\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 2. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
O I* & 1304.858 & 96.32  &     1.86  &    12.21  \\
O I** & 1306.029 & 96.21  &     2.55  &    12.51  \\
S II & 1250.584 & 99.06  &     2.82  &    13.38  \\
     & 1253.811 &  98.18  &     3.60  &    13.47  \\
Si II  & 1526.707 &  97.86  &     3.32  &    13.46 \\ 
Si II* & 1264.738 & 98.10  &     3.75  &    12.33  \\
      & 1265.002  & 97.75  &     4.09  &    12.33  \\
      & 1309.276 & 97.76  &     2.37  &    12.02  \\
      & 1533.431  & 97.65  &     2.05  &    12.18 \\
\hline
\multicolumn{5}{c}{110 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & 109.86  &     2.04  &    11.60 \\
C II* & 1335.708$^{a}$  &  110.97  &     3.73  &    13.58 \\
      & 1335.708$^{b}$  &  109.13  &     3.16  &    13.82 \\
Fe II & 1608.451 & 109.43  &     1.62  &    12.71  \\
      & 2382.765 &  108.83  &     1.50  &    13.02 \\
      & 2586.650 & 109.51  &     1.64  &    12.81 \\
      & 2600.173 & 109.33  &     1.54  &    13.00 \\
Mg I & 2852.964$^{a}$  & 111.09  &     5.00  &    10.78  \\
     & 2852.964$^{b}$  & 110.26  &     2.47  &    10.70 \\
Mg II  & 2796.352$^{a}$  & 110.20  &     2.14  &    12.62 \\
       & 2796.352$^{b}$  & 109.52  &     2.00  &    13.14 \\
       & 2803.531$^{a}$   & 110.03  &     2.30  &    12.52 \\
       & 2803.531$^{b}$   & 109.34  &     2.23  &    12.82 \\
O I & 1302.169 & 109.29  &     3.06  &    14.11 \\
S II  & 1253.811 &  108.76  &     5.00  &    13.39  \\
Si II  & 1526.707 &  109.44  &     1.92  &    12.97 \\ 
Si II* & 1264.738 & 109.76  &     2.59  &    11.78  \\
\hline
\multicolumn{5}{c}{120 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787 & 119.98  &     1.50  &    10.70: \\
C II* & 1335.708$^{a}$  & 122.52  &     5.16  &    12.46 \\
      & 1335.708$^{b}$  &  120.38  &     1.50  &    12.14 \\
Fe II & 2382.765 &  119.74  &     1.50  &    11.45 \\
      & 2586.650 & 121.24  &     1.93  &    11.75: \\
      & 2600.173 & 120.85  &     3.16  &    11.56 \\
Mg II  & 2796.352$^{a}$  & 118.28  &     3.57  &    11.15 \\
       & 2796.352$^{b}$  & 120.71  &     1.75  &    11.34 \\
       & 2803.531$^{a}$   & 120.13  &     3.87  &    11.30 \\
       & 2803.531$^{b}$   & 120.51  &     1.50  &    11.04: \\
O I & 1302.169 &  120.46  &     2.34  &    12.42 \\
S II  & 1253.811 & 120.00  &     6.00  &    13.39  \\
\hline
\multicolumn{5}{c}{127 km s$^{-1}$ Component}\\
\hline
Fe II & 2382.765 & 127.38  &     5.09  &    11.56 \\
      & 2586.650 &  128.25  &     1.50  &    11.61: \\
      & 2600.173 & 128.77  &     1.50  &    11.36: \\
Mg II  & 2796.352$^{a}$  & 125.58  &     2.81  &    11.30 \\
       & 2796.352$^{b}$  & 127.74  &     3.22  &    11.45 \\
       & 2803.531$^{a}$   & 125.55  &     1.50  &    11.30 \\
       & 2803.531$^{b}$   & 127.86  &     4.99  &    11.52 \\
\hline
\multicolumn{5}{l}{$^a$ 1997 \qquad $^b$ 1999}\\
\multicolumn{5}{l}{Notes---Units for velocity v, dispersion b, and}\\ 
\multicolumn{5}{l}{column density N are, respectively, km~s$^{-1}$,}\\ 
\multicolumn{5}{l}{km~s$^{-1}$, and cm$^{-2}$. Column densities that}\\
\multicolumn{5}{l}{are more uncertain because of weak, blended,}\\ 
\multicolumn{5}{l}{or saturated components are marked with }\\ 
\multicolumn{5}{l}{colons. Error estimates are provided in the}\\
\multicolumn{5}{l}{text.}\\
\end{tabular}
}


%\documentclass[10pt]{paastex}
%\usepackage{myemulateapj5}
%\pagestyle{empty}
%\begin{document}
\clearpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. HD 93205}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\multicolumn{5}{c}{$-$142 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & $-$141.68  &     4.17  &    11.80 \\
      & 1670.787$^{b}$ & $-$142.66  &     4.33  &    11.80  \\
C II & 1334.532 & $-$142.00  &     5.43  &    13.84 \\
Fe II & 1608.451 & $-$142.11  &     2.83  &    12.72  \\
      & 2382.765 & $-$143.44  &     3.35  &    12.82 \\
      & 2586.650 & $-$142.58  &     3.33  &    12.86 \\
      & 2600.173 & $-$143.00  &     3.41  &    12.82 \\
Mg I & 2852.964 & $-$142.15  &     4.19  &    10.85  \\
Mg II & 2796.352 & $-$142.36  &     3.36  &    12.73 \\
      & 2803.531 & $-$141.72  &     3.46  &    12.68 \\
O I & 1302.169 & $-$142.06  &     3.42  &    12.97  \\
O I** & 1306.029 & $-$141.67  &     2.13  &    12.09  \\
S II & 1259.519 & $-$142.18  &     6.90  &    13.17  \\
Si II & 1304.370 & $-$141.86  &     3.60  &    12.97  \\
     & 1526.707 & $-$142.06  &     3.42  &    12.97  \\
Si II* & 1264.738 & $-$142.57  &     4.63  &    11.92  \\
%       &     &     &     &     \\
C IV & 1548.195 &  $-$128.91  &     5.00  &    11.99 \\
     & 1550.770 & $-$133.50  &     3.96  &    11.81  \\
\hline
\multicolumn{5}{c}{$-$98 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & $-$98.89  &     5.04  &    12.44 \\
      & 1670.787$^{b}$ & $-$98.34  &     6.81  &    12.60  \\
Fe II & 1608.451 & $-$98.18  &     5.65  &    13.21 \\
      & 2382.765 & $-$100.41  &     4.76  &    13.19 \\
      & 2586.650 & $-$98.71  &     5.43  &    13.26 \\
      & 2600.173 & $-$99.63  &     4.87  &    13.23 \\
Mg I & 2852.964 & $-$98.21  &     4.41  &    11.72 \\
Mn II & 2576.877 & $-$98.00  &     5.37  &    11.34 \\
      & 2594.499 & $-$99.96  &     2.19  &    11.46 \\
      & 2606.462 & $-$99.51  &     4.76  &    11.65 \\
O I** & 1306.029 & $-$99.63  &     1.50  &    12.09: \\
S II  & 1250.584 & $-$97.93  &     5.74  &    14.03 \\
      & 1253.811 & $-$97.51  &     6.34  &    14.01  \\
      & 1259.519 & $-$98.93  &     5.28  &    13.93  \\
Si II & 1304.370 & $-$98.56  &     5.19  &    14.00 \\
      & 1526.707 & $-$99.67  &     4.50  &    13.89 \\
Si II* & 1264.738  & $-$98.31  &     3.69  &    12.11 \\
      & 1309.276 & $-$98.00  &     3.58  &    12.10  \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$102.52  &     7.00  &    11.49 \\
       & 1862.790 & $-$97.39  &     9.98  &    11.89  \\
C IV & 1548.195 &  $-$100.26  &     8.85  &    12.72 \\
     & 1550.770 & $-$99.62  &     6.85  &    12.64  \\
Si IV  & 1402.770 & $-$99.40  &     3.44  &    11.89  \\
\hline
\multicolumn{5}{c}{$-$89 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & $-$89.00  &     1.59  &    14.50: \\
      & 1670.787$^{b}$ & $-$89.00  &     2.17  &    13.79: \\
Fe II & 1608.451 &  $-$88.89  &     2.11  &    13.70: \\
      & 1611.201 & $-$86.04  &     5.85  &    14.21 \\
      & 2382.765 & $-$90.16  &     1.77  &    14.11: \\
      & 2586.650 & $-$90.19  &     1.50  &    13.60: \\
      & 2600.173 & $-$89.00  &     3.24  &    13.71:  \\
Mg I & 1827.935 & $-$86.04  &     8.48  &    12.76:   \\
     & 2852.964 & $-$89.23  &     2.54  &    11.94 \\
Mn II & 2576.877 & $-$89.00  &     3.66  &    11.88 \\
   \end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
   & 2594.499 & $-$90.44  &     1.63  &    11.63  \\
Ni II & 1370.132 & $-$90.29  &     3.00  &    12.42 \\
O I** & 1306.029 & $-$89.15  &     2.80  &    13.17  \\
S II & 1250.584 & $-$88.59  &     3.12  &    14.07 \\
     & 1253.811 &  $-$88.77  &     2.84  &    14.09 \\
     & 1259.519 & $-$89.12  &     3.32  &    14.13  \\
Si II & 1304.370 & $-$89.00  &     3.72  &    14.14:  \\
      & 1526.707 & $-$89.00  &     4.66  &    14.09:  \\
      & 1808.013 & $-$89.07  &     2.63  &    14.19  \\
Si II* & 1264.738 & $-$88.00  &     3.45  &    12.87  \\
       & 1309.276 & $-$88.45  &     3.07  &    12.62  \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$89.72  &     7.50  &    12.18 \\
       & 1862.790 & $-$87.55  &     5.73  &    11.95  \\
C IV & 1548.195 &  $-$89.97  &     6.86  &    12.57 \\
     & 1550.770 & $-$88.82  &     4.86  &    12.43  \\
Si IV & 1402.770 & $-$91.54  &     4.21  &    12.07  \\
\hline
\multicolumn{5}{c}{$-$83 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & $-$83.00  &     4.06  &    12.66: \\
      & 1670.787$^{b}$ & $-$83.00  &     3.71  &    12.52: \\
Fe II & 1608.451 &  $-$82.94  &     2.41  &    13.84  \\
      & 2382.765 & $-$86.33  &     6.76  &    13.66: \\
      & 2586.650 &  $-$84.66  &     4.21  &    13.90: \\
      & 2600.173 & $-$83.00  &     4.67  &    13.39:  \\
Mg I & 2852.964 & $-$83.17  &     1.97  &    12.19  \\
Mn II & 2576.877 & $-$83.02  &     2.64  &    11.86  \\
      & 2594.499 & $-$84.15  &     3.80  &    12.10 \\
      & 2606.462 & $-$86.48  &     5.31  &    12.13:  \\
Ni II & 1317.217$^{c}$ &  $-$85.07  &     5.13  &    12.71: \\
      &  1317.217$^{d}$ & $-$85.15  &     5.21  &    12.66: \\
      & 1370.132 & $-$84.14  &     3.00  &    12.66  \\
      & 1709.600 & $-$85.39  &     4.10  &    12.58:  \\
      & 1741.549 & $-$84.56  &     5.59  &    12.90:  \\
      & 1751.910 & $-$85.39  &     4.61  &    12.67:  \\
O I** & 1306.029 &   $-$83.21  &     2.03  &    13.26 \\
S I & 1425.030 & $-$84.14  &     2.13  &    12.00 \\
S II & 1250.584 & $-$82.22  &     2.07  &    14.12  \\
     & 1253.811 & $-$82.61  &     2.55  &    14.13  \\
     & 1259.519 & $-$83.05  &     1.85  &    14.05  \\
Si II & 1304.370 & $-$83.00  &     5.16  &    14.13:  \\
      & 1526.707 &  $-$83.00  &     5.93  &    13.97: \\
     & 1808.013 & $-$83.02  &     2.46  &    14.22  \\
Si II* & 1264.738 &  $-$83.00  &     3.54  &    12.73 \\
      & 1309.276 & $-$82.94  &     1.92  &    12.69  \\
\hline
\multicolumn{5}{c}{$-$75 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & $-$74.11  &     3.00  &    11.34  \\
      & 1670.787$^{b}$ & $-$74.91  &     3.22  &    11.43  \\
Mg I & 2852.964 & $-$75.00  &     5.07  &    11.08  \\
Mg II & 2803.531 & $-$71.07  &     3.00  &    12.12: \\
S II & 1259.519 & $-$78.46  &     2.40  &    13.31  \\
Si II & 1304.370 & $-$72.34  &     3.00  &    12.68 \\
      & 1526.707 & $-$71.31  &     3.00  &    12.34: \\
\hline
\multicolumn{5}{c}{$-$66 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & $-$65.40  &     1.84  &    12.28 \\
      & 1670.787$^{b}$ & $-$66.44  &     2.61  &    12.20 \\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Fe II & 1608.451 & $-$65.37  &     1.57  &    13.47 \\
      & 2382.765 & $-$66.17  &     2.42  &    13.35 \\
      & 2586.650 &  $-$65.66  &     1.76  &    13.51  \\
      & 2600.173 & $-$65.91  &     2.11  &    13.52   \\
Mg I & 2852.964 &  $-$65.56  &     1.76  &    11.11  \\
Mg II & 2803.531 & $-$65.21  &     1.95  &    13.94:  \\
Mn II & 2576.877 & $-$65.63  &     3.68  &    11.70 \\
      & 2594.499 & $-$65.08  &     4.50  &    11.72  \\
      & 2606.462 & $-$66.99  &     3.06  &    11.45  \\
Ni II & 1317.217$^{c}$ & $-$63.64  &     4.48  &    12.43  \\
      & 1370.132 &  $-$64.57  &     3.15  &    12.53  \\
      & 1741.549 & $-$64.46  &     2.15  &    12.45  \\
S II & 1250.584 & $-$64.45  &     1.55  &    13.30  \\
     & 1253.811 & $-$65.33  &     4.42  &    13.57 \\
     & 1259.519 & $-$65.66  &     2.36  &    13.43  \\
Si II & 1304.370 & $-$65.21  &     2.33  &    13.59 \\
      & 1526.707 &  $-$65.36  &     2.00  &    13.74  \\
      & 1808.013 & $-$62.75  &     6.33  &    13.95:  \\
Si II* & 1264.738 & $-$65.96  &     2.00  &    10.90  \\
\hline
\multicolumn{5}{c}{$-$58 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ &  $-$60.00  &     6.00  &    11.80 \\
      & 1670.787$^{b}$ &  $-$59.85  &     3.00  &    11.59 \\
Fe II  & 2382.765 & $-$58.86  &     3.04  &    12.78  \\
      & 2586.650 & $-$57.76  &     3.96  &    12.90 \\
      & 2600.173 & $-$58.55  &     3.00  &    12.76  \\
Si II & 1304.370 & $-$59.00  &     5.00  &    13.14:  \\
      & 1526.707 & $-$59.00  &     5.00  &    13.08:  \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$61.55  &     4.55  &    11.60  \\
       & 1862.790 & $-$62.12  &     4.56  &    11.65  \\
C IV & 1548.195 &  $-$60.47  &     6.74  &    13.19 \\
     & 1550.770 & $-$60.61  &     6.75  &    13.20  \\
Si IV & 1393.755 & $-$60.60  &     6.15  &    12.63  \\
      & 1402.770 & $-$61.12  &     6.34  &    12.67  \\
\hline
\multicolumn{5}{c}{$-$53 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ &  $-$53.13  &     3.55  &    11.99 \\
      & 1670.787$^{b}$ & $-$54.15  &     3.71  &    12.03  \\
Fe II & 1608.451 & $-$54.34  &     6.29  &    13.21: \\
      & 2382.765 & $-$53.78  &     1.70  &    13.19 \\
      & 2586.650 & $-$52.61  &     1.50  &    12.86  \\
      & 2600.173 & $-$53.21  &     2.05  &    12.97  \\
Mg I & 2852.964 & $-$54.43  &     3.55  &    10.85 \\
Mn II & 2576.877 &  $-$55.00  &     3.52  &    11.36: \\
Ni II & 1370.132 & $-$52.27  &     3.07  &    12.41: \\
S II & 1250.584 & $-$54.26  &     1.91  &    13.34 \\
     & 1253.811 & $-$53.28  &     3.48  &    13.64 \\
     & 1259.519 &  $-$54.81  &     3.78  &    13.72  \\
Si II & 1304.370 & $-$54.14  &     2.60  &    13.50  \\
      & 1526.707 & $-$54.56  &     2.42  &    13.60  \\
      & 1808.013 & $-$52.95  &     1.50  &    13.58  \\
\hline
\multicolumn{5}{c}{$-$35 km s$^{-1}$ Component}      \\
\hline
Cl I & 1347.240 & $-$36.05  &     5.58  &    12.03  \\
Cu II & 1358.773 & $-$33.42  &     6.41  &    11.95 \\
Fe II & 1608.451 & $-$34.09  &     7.47  &    14.58: \\
      & 1611.201 & $-$34.69  &     6.17  &    14.76 \\
Ga II & 1414.402 &  $-$36.66  &     7.62  &    11.23 \\
\\
\end{tabular}
%
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Ge II & 1237.059 &  $-$33.93  &     8.21  &    11.79 \\
Mg I & 1747.794 & $-$36.51  &     4.16  &    12.97 \\
     & 1827.935 & $-$35.82  &     8.50  &    13.18   \\
     & 2852.964 & $-$35.01  &     4.94  &    14.03:  \\
Mg II & 1239.925 & $-$34.81  &     7.32  &    15.63 \\
      & 1240.395 & $-$35.16  &     7.28  &    15.65 \\
Mn II & 2576.877 & $-$34.85  &     7.23  &    13.09  \\
      & 2594.499 & $-$34.71  &     7.07  &    13.10  \\
      & 2606.462 & $-$35.25  &     7.37  &    13.08   \\
Ni II & 1317.217$^{c}$ & $-$31.94  &     5.81  &    13.37  \\
      & 1317.217$^{d}$ & $-$33.53  &     6.49  &    13.42  \\
      & 1370.132 & $-$32.59  &     4.58  &    13.33 \\
      & 1454.842 & $-$32.74  &     3.83  &    12.81 \\
      & 1709.600 & $-$32.39  &     5.27  &    13.44 \\
      & 1741.549 & $-$32.43  &     5.98  &    13.49  \\
      & 1751.910 & $-$31.74  &     5.55  &    13.45  \\
O I** & 1306.029 & $-$36.22  &     5.41  &    14.28 \\
S I & 1425.030 & $-$36.42  &     9.48  &    12.41 \\
S II & 1250.584 & $-$33.76  &     6.96  &    15.82:  \\
Si II & 1808.013 & $-$34.51  &     7.10  &    15.97: \\
Si II* & 1265.002 & $-$35.83  &     5.72  &    14.56: \\
       & 1309.276 & $-$35.82  &     5.55  &    14.31: \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$35.81  &     8.03  &    13.78:  \\
       & 1862.790 & $-$35.46  &     7.93  &    13.81: \\
C IV & 1548.195 &  $-$34.85  &     7.83  &    14.31: \\
     & 1550.770 & $-$34.83  &     7.87  &    14.32:  \\
Si IV & 1393.755 & $-$33.39  &     7.60  &    14.81:  \\
      & 1402.770 & $-$34.69  &     7.18  &    14.91:  \\
\hline
\multicolumn{5}{c}{$-$18 km s$^{-1}$ Component} \\
\hline
Cu II & 1358.773 & $-$18.08  &     3.08  &    11.95  \\
Fe II & 1611.201 & $-$18.36  &     3.03  &    14.72 \\
Ga II & 1414.402 &  $-$18.90  &     2.79  &    11.11 \\
Ge II & 1237.059 & $-$18.68  &     2.31  &    11.78 \\
Mg I & 1747.794 & $-$18.00  &     2.65  &    12.77: \\
     & 1827.935 & $-$18.69  &     6.00  &    12.68   \\
     & 2852.964 & $-$18.00  &     3.22  &    12.32: \\
Mg II & 1239.925 & $-$18.09  &     3.11  &    15.50 \\
      & 1240.395 & $-$18.28  &     3.17  &    15.54 \\
Mn II & 2576.877 & $-$18.75  &     2.55  &    13.92  \\
      & 2594.499 & $-$18.88  &     2.54  &    13.82 \\
      & 2606.462 & $-$19.33  &     3.45  &    13.40  \\
Ni II & 1317.217$^{c}$ & $-$14.55  &     5.66  &    13.17  \\
      & 1317.217$^{d}$ & $-$15.88  &     4.76  &    13.07  \\
      & 1370.132 & $-$15.98  &     5.00  &    13.07 \\
      & 1454.842 & $-$14.85  &     4.97  &    12.54 \\
      & 1709.600 & $-$15.74  &     5.45  &    13.21 \\
      & 1741.549 & $-$14.93  &     5.80  &    13.22  \\
      & 1751.910 & $-$13.97  &     5.29  &    13.24 \\
O I] & 1355.598 & $-$18.31  &     2.62  &    17.44 \\
O I** & 1306.029 & $-$18.31  &     3.82  &    13.00 \\
S II & 1250.584 & $-$17.62  &     3.61  &    15.53  \\
Si II & 1808.013 & $-$18.13  &     3.12  &    15.50 \\
Si II* & 1265.002 & $-$15.09  &     2.24  &    12.79 \\
       & 1309.276 & $-$16.34  &     8.24  &    12.57 \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$18.00  &     8.00  &    12.21  \\
       & 1862.790 & $-$18.00  &     4.73  &    11.99 \\
\end{tabular}
}
\newpage
%
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline

%            &     &     &     &     \\
%	          &     &     &     &     \\
%		        &     &     &     &     \\
C IV & 1548.195 &  $-$18.00  &     9.40  &    13.14 \\
     & 1550.770 & $-$18.00  &     9.41  &    13.14 \\
Si IV & 1393.755 & $-$18.00  &     8.22  &    12.49  \\
      & 1402.770 & $-$18.00  &     5.04  &    12.68  \\
\hline
\multicolumn{5}{c}{$-$3 km s$^{-1}$ Component}\\
\hline
Cl I & 1347.240 & $-$2.78  &     2.50  &    12.69  \\ 
Cu II & 1358.773 &  $-$3.15  &     6.17  &    12.07  \\
Fe II & 1611.201 & $-$3.51  &     5.81  &    14.94 \\
Ga II & 1414.402 &  $-$3.95  &     7.87  &    11.36 \\
Ge II & 1237.059 & $-$1.75  &     7.95  &    11.93 \\
Mg I & 1747.794 & $-$2.84  &     7.53  &    13.41 \\
     & 1827.935 & $-$4.29  &     3.76  &    13.15  \\
     & 2852.964 & $-$3.40  &     6.29  &    13.55: \\
Mg II & 1239.925 & $-$2.68  &     6.32  &    15.79 \\
      & 1240.395 & $-$2.15  &     7.15  &    15.83 \\
Mn II & 2576.877 & $-$3.80  &     6.18  &    13.34:  \\
      & 2594.499 & $-$3.93  &     6.42  &    13.32 \\
      & 2606.462 & $-$3.95  &     6.69  &    13.33  \\
Ni II & 1317.217$^{c}$ & $-$2.88  &     4.13  &    13.46 \\
      & 1317.217$^{d}$ & $-$3.73  &     4.98  &    13.48 \\
      & 1370.132 &  $-$2.90  &     5.56  &    13.61 \\
      & 1454.842 & $-$3.78  &     4.20  &    13.17 \\
      & 1709.600 & $-$2.67  &     4.97  &    13.64 \\
      & 1741.549 & $-$3.30  &     4.05  &    13.56  \\
      & 1751.910 &  $-$2.02  &     4.88  &    13.65 \\
O I] & 1355.598 & $-$2.96  &     6.77  &    17.41 \\
S I & 1295.653 & $-$3.03  &     1.50  &    11.92: \\
   & 1425.030 &  $-$4.57  &     5.24  &    12.20  \\
S II & 1250.584 & $-$3.40  &     5.58  &    15.96:  \\
Si II & 1808.013 & $-$3.40  &     7.37  &    15.75: \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$4.28  &     5.61  &    12.45  \\
       & 1862.790 & $-$3.97  &     6.66  &    12.58 \\
C IV & 1548.195 &   $-$3.00  &     8.00  &    13.06 \\
     & 1550.770 & $-$3.00  &     7.50  &    13.03 \\
Si IV & 1393.755 &  $-$3.00  &     8.00  &    12.34  \\
      & 1402.770 & $-$3.00  &     8.00  &    12.47 \\
\hline
\multicolumn{5}{c}{8 km s$^{-1}$ Component}\\
\hline
Cl I & 1347.240 & 7.36  &     3.94  &    13.95 \\ 
Cu II & 1358.773 &   7.71  &     3.07  &    12.13  \\
Fe II & 1611.201 & 7.81  &     4.12  &    15.01 \\
Ga II & 1414.402 &  7.98  &     3.87  &    11.46 \\
Ge II & 1237.059 & 8.25  &     3.54  &    12.04 \\
Mg I & 1747.794 & 7.41  &     4.00  &    13.62 \\
     & 1827.935 & 6.38  &     4.09  &    13.70  \\
     & 2852.964 & 7.80  &     4.82  &    13.21: \\
Mg II & 1239.925 & 8.77  &     4.00  &    15.88 \\
      & 1240.395 & 8.78  &     3.71  &    15.88 \\
Mn II & 2576.877 & 7.20  &     4.51  &    13.64:  \\
      & 2594.499 & 7.37  &     4.59  &    13.51 \\
      & 2606.462 & 7.09  &     4.47  &    13.52  \\
Ni II & 1317.217$^{c}$ &  8.31  &     6.25  &    13.69 \\
      & 1317.217$^{d}$ & 7.86  &     5.58  &    13.62 \\
      & 1370.132 &  8.55  &     4.85  &    13.65 \\
      & 1454.842 & 7.43  &     5.83  &    13.41 \\
      & 1709.600 & 8.37  &     5.29  &    13.77 \\
      & 1741.549 & 7.95  &     6.34  &    13.83  \\
\end{tabular}
%
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
      & 1751.910 &   9.24  &     5.31  &    13.75 \\
O I] & 1355.598 &  7.97  &     3.87  &    17.70 \\
S I & 1295.653 & 8.40  &     2.38  &    12.53 \\
   & 1425.030 &  7.53  &     1.67  &    12.33 \\
S II & 1250.584 & 7.80  &     6.44  &    15.83:  \\
Si II & 1808.013 & 7.80  &     4.78  &    15.89: \\
Si II* & 1264.738 & 8.22  &     2.00  &    11.30  \\
%       &     &     &     &     \\
Al III & 1854.716 &  7.21  &     7.84  &    12.77  \\
       & 1862.790 & 7.68  &     6.75  &    12.70 \\
C IV & 1548.195 &  8.00  &     7.37  &    13.01 \\
     & 1550.770 & 8.00  &     7.81  &    13.04 \\
Si IV & 1393.755 & 8.00  &     7.79  &    12.41  \\
      & 1402.770 &  8.00  &     7.18  &    12.38 \\
\hline
\multicolumn{5}{c}{18 km s$^{-1}$ Component}\\
\hline
Fe II & 2586.650 &  22.76  &     1.71  &    13.15: \\
Mg I & 2852.964 & 18.00  &     5.00  &    11.90:  \\
Mn II & 2576.877 & 18.00  &     2.49  &    11.93  \\
      & 2594.499 &  18.00  &     4.47  &    12.03 \\
      & 2606.462 & 18.00  &     6.22  &    12.14 \\
Ni II  & 1370.132 &  18.27  &     1.50  &    12.36 \\
      & 1709.600 &  19.52  &     3.02  &    12.70 \\
S II & 1250.584 & 18.00  &     2.44  &    14.27: \\
Si II & 1808.013 & 18.00  &     2.70  &    14.30 \\
%       &     &     &     &     \\
Al III & 1854.716 &  18.00  &     2.97  &    11.20  \\
       & 1862.790 & 18.00  &     5.84  &    11.82 \\
C IV & 1548.195 &  18.00  &     5.01  &    12.61 \\
     & 1550.770 & 18.00  &     5.14  &    12.44 \\
Si IV & 1393.755 & 18.00  &     5.00  &    11.83 \\
      & 1402.770 &  18.00  &     7.51  &    12.18 \\
\hline
\multicolumn{5}{c}{27 km s$^{-1}$ Component}\\
\hline
Cu II & 1358.773 &  27.21  &     2.36  &    11.34:  \\
Fe II & 1608.451 &  27.45  &     1.50  &    12.95  \\
      & 2586.650 & 27.02  &     1.50  &    13.16 \\
Mg I & 2852.964 &  25.90  &     2.77  &    11.38 \\
Mn II & 2576.877 & 24.48  &     3.50  &    11.57  \\
      & 2594.499 &  27.00  &     7.55  &    11.73 \\
Ni II  & 1370.132 & 24.81  &     7.00  &    12.60 \\
      & 1751.910 & 24.09  &     4.10  &    12.63 \\
S II & 1250.584 &  23.21  &     4.07  &    13.94 \\
Si II & 1808.013 & 25.11  &     4.00  &    13.87 \\
%       &     &     &     &     \\
C IV & 1548.195 &  26.12  &     3.64  &    12.18 \\
     & 1550.770 &  27.00  &     8.84  &    12.62 \\
Si IV & 1393.755 & 27.80  &     7.00  &    11.43 \\
\hline
\multicolumn{5}{c}{35 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 36.24  &     7.99  &    11.65 \\
      & 1670.787$^{b}$ &  35.08  &     4.92  &    11.43 \\
C II* & 1335.708 &  36.07  &     7.68  &    13.46:  \\
Fe II  & 1608.451 & 35.68  &     1.50  &    12.18: \\
      & 2382.765 & 34.69  &     5.31  &    12.33  \\
      & 2586.650 & 33.64  &     4.63  &    12.39 \\
      & 2600.173 & 35.88  &     1.99  &    11.83 \\
Mg I  & 2852.964 & 34.21  &     1.82  &    10.48  \\
Mg II & 2803.531 & 35.00  &     7.36  &    13.14:  \\
Si II & 1526.707 & 34.22  &     6.47  &    13.13  \\
%       &     &     &     &     \\
C IV & 1548.195 &  35.00  &     7.00  &    12.25 \\
     & 1550.770 & 35.00  &     1.85  &    11.58 \\
\end{tabular}
}
\newpage
%           &     &     &     &     \\
%	         &     &     &     &     \\
%		       &     &     &     &     \\
%
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\multicolumn{5}{c}{47 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ &  48.53  &     1.50  &    10.78 \\
      & 1670.787$^{b}$ &  45.92  &     3.94  &    11.26  \\
C II* & 1335.708 & 47.38  &     2.11  &    13.36 \\
Fe II & 1608.451 & 47.36  &     1.50  &    12.18 \\
      & 2382.765 & 47.07  &     1.50  &    12.10 \\
      & 2586.650 &  47.50  &     1.50  &    12.13  \\
      & 2600.173 &  47.35  &     1.50  &    12.00  \\
Mg I & 2852.964 & 47.47  &     1.50  &    10.60 \\
Mg II & 2796.352 & 47.10  &     2.21  &    12.36  \\
      & 2803.531 & 45.33  &     4.25  &    12.55  \\
Si II  & 1526.707 & 44.11  &     5.33  &    12.77  \\
\hline
\multicolumn{5}{c}{69 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 69.23  &     3.53  &    11.18 \\
      & 1670.787$^{b}$ &   69.24  &     6.58  &    11.53 \\
C II & 1334.532 & 68.96  &     8.06  &    13.87  \\
C II* & 1335.708 & 69.44  &     5.38  &    13.12 \\
Fe II & 1608.451 & 67.78  &     2.04  &    12.18 \\
      & 2382.765 & 68.01  &     4.69  &    12.26 \\
      & 2586.650 &  68.18  &     5.73  &    12.31  \\
      & 2600.173 & 67.84  &     3.95  &    12.17 \\
Mg II & 2796.352 & 68.57  &     5.38  &    12.34 \\
      & 2803.531 & 68.35  &     5.56  &    12.34 \\
O I & 1302.169 & 68.66  &     5.54  &    12.63  \\
Si II  & 1526.707 & 68.66  &     5.54  &    12.63 \\
\hline
\multicolumn{5}{c}{80 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 79.19  &     3.52  &    11.60 \\
      & 1670.787$^{b}$ &    78.96  &     2.80  &    11.53 \\
C II & 1334.532 & 80.00  &     5.80  &    13.88: \\
C II* & 1335.708 & 78.76  &     3.36  &    13.28 \\
Fe II & 1608.451 & 79.94  &     2.81  &    12.58 \\
      & 2382.765 & 79.26  &     3.49  &    12.71 \\
      & 2586.650 &  79.86  &     3.45  &    12.70  \\
      & 2600.173 & 79.46  &     3.35  &    12.71 \\
Mg II & 2796.352 & 79.92  &     3.53  &    12.63 \\
      & 2803.531 & 79.84  &     3.56  &    12.62 \\
O I & 1302.169 & 79.79  &     3.85  &    12.88 \\
Si II  & 1526.707 & 79.79  &     3.85  &    12.88 \\
%       &     &     &     &     \\
C IV & 1548.195 &  82.42  &     2.79  &    11.92 \\
     & 1550.770 & 83.59  &     3.00  &    11.87 \\
\hline
\multicolumn{5}{c}{88 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 87.20  &     6.08  &    11.51 \\
      & 1670.787$^{b}$ &  86.46  &     4.45  &    11.53 \\
C II & 1334.532 & 88.00  &     4.36  &    13.97: \\
C II* & 1335.708 & 86.18  &     4.56  &    13.53 \\
Fe II & 1608.451 &  87.72  &     1.74  &    12.26 \\
      & 2382.765 &  87.57  &     2.65  &    12.30 \\
      & 2586.650 &  88.31  &     2.68  &    12.18  \\
      & 2600.173 & 87.64  &     2.43  &    12.26  \\
Mg II & 2796.352 & 88.26  &     3.72  &    12.36 \\
      & 2803.531 & 87.86  &     3.71  &    12.38 \\
O I & 1302.169 & 88.29  &     3.02  &    12.69 \\
       &     &     &     &     \\
\end{tabular}
%
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Si II  & 1526.707 & 88.29  &     3.02  &    12.69 \\
Si II* & 1264.738 & 85.52  &     6.00  &    11.43  \\
C IV & 1548.195 & 91.94  &     4.04  &    12.05 \\
     & 1550.770 & 95.43  &     6.00  &    12.49 \\
Si IV & 1393.755 & 91.31  &     7.51  &    11.90  \\
\hline
\multicolumn{5}{c}{100 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 100.23  &     3.49  &    12.18 \\
      & 1670.787$^{b}$ &   99.68  &     4.82  &    12.29 \\
Fe II & 1608.451 &  99.60  &     2.88  &    13.15 \\
      & 2382.765 & 99.63  &     3.41  &    13.34 \\
      & 2586.650 & 99.33  &     2.93  &    13.16  \\
      & 2600.173 & 99.80  &     3.49  &    13.25  \\
Mg I & 2852.964 & 99.95  &     3.56  &    11.23  \\
Mg II & 2803.531 &  99.74  &     3.89  &    13.17 \\
Mn II & 2606.462 & 99.09  &     3.96  &    11.32:  \\
S II & 1250.584  & 100.00  &     5.97  &    13.47: \\
     & 1253.811 &  100.00  &     3.34  &    13.12  \\
Si II  & 1526.707 & 99.69  &     3.53  &    13.44 \\
Si II* & 1264.738 & 100.02  &     3.31  &    12.01  \\
%      &     &     &     &     \\
\hline
\multicolumn{5}{c}{108 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 108.64  &     3.39  &    12.05 \\
      & 1670.787$^{b}$ &  107.54  &     1.96  &    11.88 \\
Fe II & 1608.451 & 107.99  &     2.69  &    13.06 \\
      & 2382.765 & 107.12  &     1.50  &    13.14 \\
      & 2586.650 & 107.96  &     3.43  &    13.16  \\
      & 2600.173 & 107.29  &     1.78  &    12.98  \\
Mg I & 2852.964 & 108.33  &     3.00  &    10.90  \\
Mg II & 2803.531 & 108.64  &     3.54  &    13.14 \\
S II & 1250.584  & 108.00  &     4.00  &    13.41 \\
     & 1253.811 &  108.00  &     3.74  &    13.36 \\
Si II  & 1526.707 & 108.54  &     3.41  &    13.46 \\
Si II* & 1264.738 & 107.82  &     4.00  &    11.69  \\
%       &     &     &     &     \\
C IV & 1548.195 &  104.31  &     9.91  &    12.47 \\
     & 1550.770 & 108.56  &     5.00  &    12.18  \\
Si IV & 1393.755 & 104.16  &     3.71  &    11.38  \\
\hline
\multicolumn{5}{c}{113 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 113.71  &     2.15  &    11.67 \\
      & 1670.787$^{b}$ &  111.54  &     1.68  &    11.72 \\
Fe II & 1608.451 & 113.58  &     1.93  &    12.78 \\
      & 2382.765 & 112.64  &     4.89  &    13.24: \\
      & 2586.650 & 113.41  &     1.54  &    12.72  \\
      & 2600.173 & 113.43  &     4.98  &    13.19  \\
Mg I & 2852.964 & 113.00  &     3.00  &    10.78  \\
Mg II & 2803.531 & 113.93  &     1.56  &    12.69 \\
Si II  & 1526.707 & 114.12  &     1.95  &    13.03 \\
Si II* & 1264.738 & 113.00  &     3.00  &    11.38  \\
\hline
\multicolumn{5}{c}{118 km s$^{-1}$ Component}\\
\hline
Al II & 1670.787$^{a}$ & 118.72  &     2.91  &    12.21 \\
      & 1670.787$^{b}$ &  117.28  &     3.55  &    12.22 \\
Fe II & 1608.451 & 118.58  &     2.13  &    13.20 \\
      & 2382.765 & 117.86  &     1.50  &    14.11:  \\
      & 2586.650 & 117.97  &     2.23  &    13.22  \\
      & 2600.173 &  118.45  &     1.50  &    13.53  \\
\end{tabular}
}
\newpage
%
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 3. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Mg I & 2852.964 & 118.48  &     2.61  &    11.08 \\
Mg II & 2803.531 & 118.65  &     2.40  &    13.29 \\
Mn II & 2576.877 & 118.11  &     1.50  &    11.08:  \\
      & 2594.499 & 116.83  &     1.71  &    11.28  \\
      & 2606.462 & 117.62  &     3.01  &    11.20  \\
Ni II & 1370.132 & 120.05  &     5.00  &    12.48:  \\
O I* & 1304.858 & 117.65  &     4.81  &    12.57  \\
O I** & 1306.029 &  119.82  &     3.04  &    12.17  \\
S II & 1250.584 & 119.00  &     5.26  &    13.54  \\
     & 1253.811 & 118.44  &     4.36  &    13.56  \\
Si II  & 1526.707 & 118.56  &     2.40  &    13.54 \\
Si II* & 1264.738 & 118.80  &     2.94  &    11.89  \\
       & 1265.002 & 118.64  &     2.84  &    12.03  \\
%       &     &     &     &     \\
C IV & 1548.195 & 118.98  &     2.80  &    11.72 \\
Si IV & 1393.755 & 117.58  &     3.45  &    11.34 \\
\hline
\multicolumn{5}{l}{$^a$ Exposure with central $\lambda$ = 1598 \AA}\\
\multicolumn{5}{l}{$^b$ Exposure with central $\lambda$ = 1763 \AA}\\
\multicolumn{5}{l}{$^c$ Exposure with central $\lambda$ = 1234 \AA}\\
\multicolumn{5}{l}{$^d$ Exposure with central $\lambda$ = 1416 \AA}\\
\multicolumn{5}{l}{Notes---Units for velocity v, dispersion b, and}\\ 
\multicolumn{5}{l}{column density N are, respectively, km~s$^{-1}$,}\\ 
\multicolumn{5}{l}{km~s$^{-1}$, and cm$^{-2}$. Column densities that}\\
\multicolumn{5}{l}{are more uncertain because of weak, blended,}\\ 
\multicolumn{5}{l}{or saturated components are marked with }\\ 
\multicolumn{5}{l}{colons. Error estimates are provided in the}\\
\multicolumn{5}{l}{text.}\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\end{tabular}
%
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. HDE 303308}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\multicolumn{5}{c}{$-$175 km s$^{-1}$ Component}\\ 
\hline
C II & 1334.532 & $-$175.19  &     2.28  &    12.31 \\
Si II &  1526.707 &  $-$177.92  &     2.81  &    11.89  \\
\hline
\multicolumn{5}{c}{$-$133 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{b}$ & $-$134.00  &     1.50  &    10.30 \\
C II & 1334.532 & $-$134.08  &     4.35  &    12.40 \\
C II* & 1335.708 & $-$133.00  &   1.80  &  11.71 \\
Fe II & 2382.765 & $-$131.37  &     3.71  &    11.15 \\
      & 2600.173 & $-$130.91  &     2.58  &    11.18 \\
Mg II & 2796.352 & $-$133.01  &     1.50  &    10.90 \\
      & 2803.531 & $-$134.76  &     5.91  &    10.90: \\
%      &  &  &  &  \\
C IV & 1548.195 & $-$129.12  &    12.00  &    12.23 \\
Si IV  & 1402.770 &  $-$136.43  &     7.55  &    11.71  \\
\hline
\multicolumn{5}{c}{$-$111 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$111.68  &     3.19  &    12.51  \\
      & 1670.787$^{b}$ & $-$112.12  &     3.93  &    12.47 \\
C II* & 1335.708 & $-$111.00  &   8.44  & 14.54:  \\
Fe II & 1608.451 & $-$111.48  &     2.90  &    13.52 \\
      & 2382.765 & $-$110.31  &     4.32  &    13.73: \\
      & 2586.650 & $-$111.54  &     2.92  &    13.53 \\
      & 2600.173 & $-$111.62  &     3.58  &    13.51: \\
Mg I & 2852.964 & $-$110.89  &     3.99  &    11.59 \\
Mg II & 2796.352 & $-$111.00  &     4.13  &    13.55: \\
      & 2803.531 & $-$111.00  &     3.75  &    13.42: \\
Mn II & 2576.877 & $-$112.56  &     3.07  &    11.46 \\
      & 2594.499 & $-$113.17  &     3.17  &    11.43 \\
      & 2606.462 & $-$107.43  &     6.63  &    11.57: \\
Ni II & 1709.600 & $-$111.16  &     2.30  &    12.35 \\
      & 1751.910 & $-$111.00  &     5.00  &    12.79 \\
O I** & 1306.029 & $-$108.97  &     7.76  &    12.73 \\
S II  & 1250.584 & $-$108.54  &     4.05  &    13.93 \\
      & 1253.811 & $-$110.50  &     3.64  &    13.66  \\
      & 1259.519 & $-$111.46  &     3.74  &    13.76  \\
Si II & 1304.370 & $-$111.04  &     3.59  &    13.86 \\
      & 1526.707 & $-$111.31  &     3.85  &    13.82 \\
Si II* & 1264.738  & $-$110.66  &     3.49  &    12.37  \\
      & 1309.276 & $-$110.86  &     3.00  &    11.86  \\
%       &  &  &  &  \\
Al III & 1854.716 & $-$106.76  &     7.78  &    11.64  \\
C IV & 1548.195 & $-$110.69  &     8.10  &    12.52 \\
     & 1550.770  & $-$111.00  &     7.35  &    12.02  \\
Si IV & 1402.770 & $-$109.55  &     6.67  &    11.92  \\
\hline
\multicolumn{5}{c}{$-$104 km s$^{-1}$ Component}\\ 
\hline
Al II  & 1670.787$^{a}$ & $-$103.89  &     3.68  &    12.45 \\
     & 1670.787$^{b}$ & $-$104.67  &     3.77  &    12.41 \\
C II* & 1335.708 & $-$104.00   &  4.51  &  14.44:  \\
Fe II & 1608.451 &  $-$103.70  &     2.74  &    13.35 \\
      & 2382.765 & $-$103.67  &     2.89  &    13.31:  \\
      & 2586.650 & $-$103.86  &     3.04  &    13.40  \\
      & 2600.173 & $-$103.89  &     3.16  &    13.35:  \\
Mg I & 2852.964 & $-$103.32  &     3.08  &    11.38    \\
Mg II & 2796.352 &  $-$104.00  &     3.85  &    13.66: \\
      & 2803.531 & $-$104.00  &     4.02  &    13.69: \\
Mn II & 2576.877 & $-$104.98  &     4.70  &    11.54 \\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
S II & 1250.584 & $-$101.87  &     1.50  &    13.32: \\
     & 1253.811 & $-$103.22  &     2.65  &    13.60 \\
     & 1259.519 & $-$104.32  &     2.65  &    13.51  \\
Si II & 1304.370 & $-$103.40  &     3.06  &    13.72  \\
      & 1526.707 & $-$103.56  &     3.07  &    13.68  \\
Si II* & 1264.738 & $-$103.73  &     2.84  &    12.19  \\
       & 1309.276 & $-$103.04  &     4.17  &    11.96  \\     
\hline
\multicolumn{5}{c}{$-$91 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$90.44  &     5.00  &    11.64 \\
     & 1670.787$^{b}$ & $-$92.03  &     5.00  &    11.65  \\
Fe II & 1608.451 &  $-$90.74  &     1.50  &    12.00:  \\
      & 2382.765 & $-$91.40  &     2.91  &    12.12  \\
      & 2586.650 & $-$90.99  &     1.72  &    12.02  \\
      & 2600.173 &  $-$90.68  &     3.41  &    12.09  \\
Mg II & 2796.352 & $-$90.00  &     3.85  &    12.50  \\
      & 2803.531 & $-$89.13  &     4.50  &    12.54  \\
Si II & 1304.370 & $-$90.17  &     4.17  &    12.73  \\
      & 1526.707 &  $-$90.28  &     3.51  &    12.68  \\
%       &  &  &  &   \\
C IV & 1548.195 & $-$92.47  &    12.00  &    13.15 \\
     & 1550.770  &  $-$95.05  &    12.00  &    13.04  \\
Si IV & 1402.770 & $-$92.00  &     8.83  &    12.74 \\
\hline
\multicolumn{5}{c}{$-$82 km s$^{-1}$ Component}\\ 
\hline
Al II    & 1670.787$^{a}$ & $-$82.19  &     1.97  &    12.22  \\
     & 1670.787$^{b}$ & $-$83.25  &     2.68  &    12.16  \\
Fe II & 1608.451 & $-$82.34  &     1.75  &    13.18 \\
      & 2382.765 &  $-$82.99  &     2.14  &    13.34 \\
      & 2586.650 &  $-$82.34  &     1.90  &    13.17  \\
      & 2600.173 &  $-$82.70  &     1.91  &    13.40  \\
Mg I & 2852.964 & $-$82.23  &     2.13  &    11.15   \\
Mg II & 1239.925 & $-$84.05  &     6.07  &    14.60  \\
Mn II & 2576.877 & $-$82.00  &     4.00  &    11.38  \\
Ni II  & 1751.910 & $-$81.36  &     3.70  &    12.76  \\
S II & 1253.811 & $-$81.97  &     1.97  &    13.21   \\
     & 1259.519  & $-$81.92  &     2.28  &    13.22  \\
Si II & 1304.370 & $-$82.38  &     2.44  &    13.29  \\
      & 1526.707 & $-$82.26  &     2.45  &    13.42  \\
Si II* & 1264.738 & $-$82.27  &     2.22  &    12.01  \\
\hline
\multicolumn{5}{c}{$-$76 km s$^{-1}$ Component}\\ 
\hline
Al II  & 1670.787$^{a}$ & $-$76.15  &     2.56  &    12.10: \\
      & 1670.787$^{b}$ & $-$76.20  &     2.99  &    12.57: \\
Fe II & 1608.451 & $-$75.99  &     2.14  &    13.17   \\
      & 2382.765 & $-$75.92  &     1.86  &    13.89:   \\
      & 2586.650 &  $-$76.04  &     2.02  &    13.18  \\
      & 2600.173 & $-$75.58  &     2.11  &    13.62   \\
Mg I & 2852.964 &  $-$76.00  &     2.54  &    11.15   \\
Mn II & 2576.877 & $-$76.00  &     6.00  &    11.20 \\
      & 2594.499 & $-$75.25  &     6.39  &    11.64:  \\
      & 2606.462 & $-$73.69  &     2.60  &    11.18:  \\
Ni II & 1317.217$^{c}$ & $-$77.33  &     5.36  &    12.31:  \\
      & 1317.217$^{d}$ & $-$75.34  &     5.81  &    12.37:  \\
S II & 1250.584 & $-$78.33  &     9.10  &    14.00:   \\
     & 1253.811 & $-$76.00  &     2.82  &    13.38  \\
     & 1259.519 & $-$76.05  &     2.55  &    13.40  \\
Si II & 1304.370 & $-$75.46  &     2.15  &    13.24:  \\
      & 1526.707 &  $-$76.23  &     1.52  &    13.32:  \\
Si II* & 1264.738 & $-$75.41  &     2.24  &    11.76:  \\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
%       &  &  &  &  \\
Al III & 1854.716 & $-$78.97  &    12.00  &    12.33  \\
       & 1862.790 & $-$79.93  &     9.00  &    11.77  \\
C IV & 1548.195 &  $-$76.37  &     7.47  &    13.19 \\
     & 1550.770 & $-$77.13  &     8.15  &    13.15  \\
Si IV & 1393.755 & $-$77.36  &     6.78  &    13.30  \\
      & 1402.770 & $-$77.44  &     5.87  &    13.28  \\
\hline
\multicolumn{5}{c}{$-$71 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ &  $-$71.54  &     5.08  &    12.46: \\
      & 1670.787$^{b}$ & $-$70.26  &     3.22  &    12.18:  \\
Fe II & 1608.451 & $-$71.06  &     5.02  &    13.30   \\
      & 2382.765 & $-$70.80  &     3.59  &    13.35:  \\
      & 2586.650 & $-$71.06  &     5.00  &    13.33  \\
      & 2600.173 & $-$70.25  &     2.79  &    13.03   \\
Mg I & 2852.964 & $-$71.00  &     5.32  &    11.51  \\
Mg II & 1239.925 & $-$72.65  &     4.04  &    14.24:  \\
Mn II & 2576.877 & $-$71.00  &     6.00  &    11.30  \\
Ni II & 1751.910 & $-$73.13  &     1.71  &    12.63:  \\
S II & 1250.584 & $-$68.88  &     6.25  &    13.47:  \\
     & 1253.811 & $-$71.00  &     3.28  &    13.49  \\
     & 1259.519 & $-$70.00  &     3.63  &    13.51  \\
Si II & 1304.370 & $-$72.46  &     6.96  &    13.93:  \\
      & 1526.707 & $-$72.41  &     5.48  &    13.79:  \\
Si II* & 1264.738 & $-$71.00  &     8.07  &    12.31:  \\
\hline
\multicolumn{5}{c}{$-$61 km s$^{-1}$ Component}\\ 
\hline
 Al II & 1670.787$^{a}$ & $-$63.03  &     4.00  &    12.08:  \\
      & 1670.787$^{b}$ &  $-$61.00  &     6.21  &    12.60: \\
Fe II & 1608.451 & $-$59.32  &     4.68  &    13.37: \\
      & 2586.650 & $-$61.00  &     3.66  &    12.96: \\
Mg I & 2852.964 &  $-$60.62  &     4.20  &    11.23 \\
S II & 1253.811 & $-$61.47  &     2.43  &    13.48  \\
     & 1259.519 & $-$58.50  &     3.50  &    13.51  \\
Si II & 1304.370 & $-$59.32  &     5.25  &    13.84  \\
      & 1526.707 & $-$60.53  &     5.68  &    13.74:  \\
Si II* & 1264.738 & $-$58.98  &     3.62  &    12.09  \\
%       &  &  &  &  \\
Al III & 1854.716 & $-$59.82  &     9.39  &    12.94  \\
      &  1862.790 & $-$58.87  &    11.31  &    12.98  \\
C IV & 1548.195 & $-$61.72  &     9.20  &    13.41 \\
     & 1550.770 & $-$59.00  &    12.00  &    13.57 \\
Si IV & 1393.755 & $-$61.22  &     5.57  &    13.31  \\
     & 1402.770 & $-$61.28  &     6.62  &    13.31  \\
\hline
\multicolumn{5}{c}{$-$54 km s$^{-1}$ Component}\\ 
\hline      
Al II & 1670.787$^{a}$ & $-$56.40  &     5.65  &    12.53: \\
Fe II  & 1611.201 & $-$50.57  &     2.72  &    13.87: \\
      & 2586.650 & $-$54.00  &     7.36  &    13.45:  \\
Mg I & 2852.964 & $-$54.50  &     5.06  &    11.28:   \\
Mn II & 2576.877 & $-$55.65  &     5.78  &    11.78  \\
      & 2594.499 & $-$53.00  &     3.88  &    11.72  \\
      & 2606.462 & $-$54.00  &     3.21  &    11.41   \\
Ni II & 1317.217$^{c}$ & $-$54.25  &     6.00  &    12.65  \\
      & 1454.842 & $-$54.00  &     6.00  &    13.04  \\
      & 1709.600 & $-$54.50  &     1.50  &    12.18:  \\
      & 1741.549 & $-$52.37  &     5.50  &    12.66  \\
      & 1751.910 & $-$54.54  &     5.00  &    12.94  \\
S II & 1250.584 & $-$55.00  &     7.49  &    14.05:  \\
     & 1253.811 & $-$54.28  &     2.50  &    13.37  \\
\\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\hline
\multicolumn{5}{c}{$-$41 km s$^{-1}$ Component}\\ 
\hline  
Cl I & 1347.240 & $-$37.58  &     5.63  &    12.67  \\
Fe II & 1611.201 & $-$41.58  &     4.17  &    14.48 \\
Mg II & 1239.925 & $-$41.60  &     6.01  &    14.88  \\
Mn II & 2576.877 & $-$41.68  &     6.53  &    12.78   \\
      & 2594.499 & $-$42.86  &     5.39  &    12.68  \\
      & 2606.462 & $-$42.47  &     6.04  &    12.71 \\
Ni II & 1317.217$^{c}$ & $-$41.47  &     5.04  &    13.35  \\
      & 1317.217$^{d}$ & $-$42.25  &     4.95  &    13.20  \\
       & 1370.132 & $-$42.37  &     3.52  &    13.07 \\
      & 1454.842 &  $-$42.15  &     4.64  &    13.40  \\
      & 1709.600 & $-$41.66  &     4.76  &    13.38  \\
      & 1741.549 & $-$42.03  &     4.47  &    13.34  \\
      & 1751.910 & $-$41.24  &     5.72  &    13.53  \\
S II & 1250.584 & $-$41.00  &     6.53  &    15.02:  \\
Si II  & 1808.013 & $-$40.30  &     7.51  &    15.19:   \\
% &  &  &  &  \\
% &  &  &  &  \\
%   &  &  &  &  \\
\hline
\multicolumn{5}{c}{$-$33 km s$^{-1}$ Component}\\ 
\hline  
Cl I  & 1347.240 & $-$29.40  &     5.42  &    12.62  \\
Fe II &  1611.201 & $-$33.53  &     3.12  &    14.42 \\
Mg II & 1239.925 & $-$32.19  &     4.91  &    15.21  \\
Mn II & 2576.877 & $-$32.74  &     4.55  &    12.85  \\
      & 2594.499 & $-$33.34  &     4.84  &    12.89  \\
      & 2606.462 &  $-$33.35  &     4.97  &    12.84 \\
Ni II & 1317.217$^{c}$ & $-$32.76  &     3.36  &    13.12  \\
      & 1317.217$^{d}$ & $-$32.18  &     5.13  &    13.32  \\
       & 1370.132 & $-$33.40  &     5.42  &    13.38   \\
      & 1454.842 &  $-$32.34  &     4.51  &    13.45  \\
      & 1709.600 & $-$32.63  &     3.92  &    13.32  \\
      & 1741.549 & $-$32.09  &     5.24  &    13.51  \\
      & 1751.910 & $-$32.12  &     3.64  &    13.37 \\
O I] & 1355.598 &  $-$32.25  &     4.34  &    16.88  \\
O I** & 1306.029 & $-$28.44  &    12.00  &    14.23  \\
S II & 1250.584 & $-$33.00  &     4.04  &    15.39: \\
Si II & 1808.013 & $-$32.89  &     4.15  &    15.33   \\
Si II* & 1309.276 & $-$36.42  &     5.18  &    13.45  \\
%       &  &  &  &  \\
Al III & 1854.716 & $-$31.60  &    11.84  &    13.81:  \\
       & 1862.790 & $-$30.91  &    10.06  &    13.93: \\
C IV & 1548.195 & $-$36.88  &    11.61  &    14.46: \\
     & 1550.770 & $-$35.85  &     9.57  &    14.62: \\
Si IV & 1393.755 & $-$37.64  &    10.09  &    14.65: \\
     & 1402.770 & $-$38.52  &    11.93  &    14.32: \\
\hline
\multicolumn{5}{c}{$-$24 km s$^{-1}$ Component}\\ 
\hline        
Cl I  & 1347.240 & $-$24.34  &     4.65  &    12.49 \\
Cu II & 1358.773 & $-$23.85  &     1.50  &    11.46  \\
Fe II &  1611.201 &  $-$24.85  &     3.31  &    14.67  \\
Ga II & 1414.402 & $-$23.07  &     2.03  &    10.90  \\
Ge II & 1237.059 & $-$22.58  &     5.38  &    11.70  \\
Mg II & 1239.925 & $-$23.78  &     3.54  &    15.31  \\
Mn II & 2576.877 & $-$23.73  &     3.73  &    13.18  \\
      & 2594.499 & $-$23.84  &     4.01  &    13.14  \\
      & 2606.462 & $-$24.22  &     4.07  &    13.15  \\
Ni II & 1317.217$^{c}$ & $-$24.66  &     5.26  &    13.40  \\
      & 1317.217$^{d}$ & $-$23.65  &     3.39  &    13.13  \\
       & 1370.132 & $-$22.30  &     6.00  &    13.39   \\
 \end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
      & 1454.842 &  $-$22.89  &     6.50  &    13.49  \\
      & 1709.600 & $-$23.11  &     5.66  &    13.50  \\
     & 1741.549 & $-$23.09  &     3.73  &    13.32  \\
      & 1751.910 & $-$23.29  &     6.00  &    13.58  \\
O I] & 1355.598 & $-$23.94  &     3.00  &    17.23  \\
S II & 1250.584 & $-$24.00  &     3.89  &    16.19:  \\ 
Si II & 1808.013 & $-$23.57  &     5.32  &    15.61 \\
Si II* & 1309.276 & $-$23.84  &     7.91  &    13.39  \\
\hline
\multicolumn{5}{c}{$-$16 km s$^{-1}$ Component}\\ 
\hline      
Cl I  & 1347.240 &  $-$16.59  &     1.50  &    11.62  \\
Fe II  &  1611.201 & $-$17.68  &     3.64  &    14.31  \\
Ga II & 1414.402 & $-$14.32  &     2.63  &    10.70  \\
Mg II & 1239.925 & $-$17.03  &     2.34  &    14.69  \\
Mn II & 2576.877 &  $-$16.00  &     4.50  &    12.50 \\
      & 2594.499 & $-$16.00  &     5.00  &    12.42  \\
      & 2606.462 & $-$16.00  &     4.50  &    12.38  \\
Ni II & 1317.217$^{c}$ & $-$14.56  &     5.20  &    13.13  \\
      & 1317.217$^{d}$ & $-$16.00  &     5.27  &    13.00  \\
       & 1370.132 &  $-$12.88  &     3.39  &    12.88  \\
      & 1454.842 &  $-$12.34  &     3.41  &    13.14  \\
      & 1709.600 &  $-$13.20  &     3.83  &    13.05  \\
      & 1741.549 & $-$13.64  &     6.70  &    13.37  \\
      & 1751.910 & $-$12.87  &     5.62  &    13.27  \\
S II & 1250.584 & $-$16.00  &     3.11  &    14.78:  \\
Si II  & 1808.013 & $-$16.00  &     1.50  &    14.13: \\ 
%      &  &  &  &  \\
C IV & 1548.195 & $-$15.00  &    11.02  &    13.34  \\ 
     & 1550.770 & $-$14.87  &    10.36  &    13.33  \\ 
Si IV & 1393.755 & $-$15.00  &    12.00  &    12.52 \\
      & 1402.770 & $-$15.00  &    12.00  &    12.50 \\ 
\hline       
\multicolumn{5}{c}{$-$3 km s$^{-1}$ Component}\\ 
\hline       
Cl I  & 1347.240 & $-$2.56  &     8.11  &    12.86  \\
Cu II & 1358.773 & $-$1.31  &     6.30  &    12.10  \\
Fe II  &  1611.201 & $-$2.17  &     7.00  &    15.03  \\
Ga II & 1414.402 & $-$3.52  &     3.02  &    10.90 \\
Ge II & 1237.059 & $-$4.69  &     6.51  &    11.92  \\
Mg II & 1239.925 & $-$3.42  &     7.47  &    15.83  \\
      & 1240.395 & $-$3.85  &     7.25  &    15.81  \\
Mn II & 2576.877 &  $-$3.00  &     6.77  &    13.48  \\
      & 2594.499 & $-$4.54  &     6.43  &    13.35  \\
      & 2606.462 &  $-$4.11  &     7.00  &    13.38  \\
Ni II & 1317.217$^{c}$ & $-$1.97  &     6.20  &    13.65  \\
      & 1317.217$^{d}$ & $-$2.40  &     5.82  &    13.58  \\
       & 1370.132 &  $-$1.71  &     5.53  &    13.63  \\
      & 1454.842 &  $-$1.52  &     6.50  &    13.71  \\
      & 1709.600 & $-$2.17  &     5.24  &    13.68  \\
      & 1741.549 & $-$1.85  &     4.68  &    13.67  \\
      & 1751.910 & $-$0.98  &     5.20  &    13.73  \\
  O I] & 1355.598 & $-$3.94  &     4.69  &    17.32  \\
O I** & 1306.029 & $-$4.91  &     5.18  &    13.20  \\
S II & 1250.584 & $-$3.00  &     6.89  &    15.93:  \\
Si II  & 1808.013 & $-$3.00  &     7.49  &    15.91:  \\
Si II* & 1309.276 & $-$5.38  &     3.19  &    12.42  \\
%       &  &  &  &  \\
Al III & 1854.716 & $-$3.00  &     7.30  &    12.49  \\
       & 1862.790 & $-$3.00  &     6.72  &    12.45 \\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\multicolumn{5}{c}{7 km s$^{-1}$ Component}\\
\hline      
Cl I  & 1347.240 & 6.58  &     2.56  &    14.74  \\
      & 1379.528 & 6.48  &     3.17  &    14.32  \\
Cu II & 1358.773 & 7.78  &     3.87  &    12.35  \\
Fe II &  1611.201 & 8.08  &     3.56  &    14.94 \\
Ga II & 1414.402 & 7.27  &     3.81  &    11.56  \\
Ge II & 1237.059 & 7.05  &     4.01  &    12.32  \\
Mg I & 1747.794 &  7.02  &     2.26  &    13.55  \\
Mg II & 1239.925 & 7.38  &     3.84  &    16.05  \\
      & 1240.395 & 7.27  &     4.13  &    16.07  \\
Mn II & 2576.877 &  7.00  &     3.73  &    13.94  \\
     & 2594.499 & 6.49  &     4.39  &    13.77  \\
      & 2606.462 &   6.49  &     3.95  &    13.81 \\
Ni II & 1317.217$^{c}$ &  9.06  &     3.97  &    13.63  \\
      & 1317.217$^{d}$ & 8.69  &     4.27  &    13.63  \\
       & 1370.132 & 9.33  &     4.43  &    13.66  \\
      & 1454.842 &  9.18  &     3.66  &    13.67  \\
      & 1709.600 & 8.64  &     4.95  &    13.82  \\
      & 1741.549 & 8.87  &     4.90  &    13.82  \\
      & 1751.910 &  9.81  &     4.38  &    13.80  \\
O I] & 1355.598 & 6.88  &     4.15  &    17.90  \\
S I & 1295.653 & 7.63  &     4.30  &    13.11  \\
    & 1425.030 & 7.89  &     4.18  &    12.94  \\
    & 1473.994 & 8.06  &     4.45  &    13.04  \\
S II & 1250.584 & 7.00  &     7.47  &    15.80:  \\
Si II  & 1808.013 &  7.00  &     5.00  &    15.90:  \\  
Si II* & 1309.276 &  5.96  &     3.16  &    11.88  \\ 
%       &  &  &  &  \\
Al III & 1854.716 &  7.00  &     7.82  &    12.76  \\
       & 1862.790 & 7.00  &     7.42  &    12.70 \\   
C IV & 1548.195 & 5.24  &    12.00  &    13.29  \\
    & 1550.770 &  6.00  &    12.00  &    13.24  \\
Si IV & 1393.755 & 5.78  &    12.00  &    12.63  \\
     & 1402.770 & 5.99  &    12.00  &    12.68  \\
\hline
\multicolumn{5}{c}{19 km s$^{-1}$ Component}\\ 
\hline                            
Fe II & 1608.451 & 22.57  &     2.18  &    13.52   \\
Ge II & 1237.059 & 19.23  &     2.94  &    11.26  \\
Mg I & 2852.964 &  23.55  &     2.46  &    11.54  \\
Mg II & 1239.925 & 17.88  &     6.50  &    14.78   \\
      & 1240.395 & 17.14  &     1.71  &    14.55  \\
Mn II & 2576.877 & 17.17  &     6.00  &    12.29   \\
      & 2594.499 & 18.38  &     5.04  &    12.12  \\
      & 2606.462 &  16.71  &     5.00  &    12.20  \\
Ni II & 1317.217$^{c}$ & 18.58  &     6.57  &    12.91  \\
    & 1317.217$^{d}$ & 18.24  &     4.74  &    12.48  \\
      & 1370.132 & 18.19  &     2.23  &    12.47   \\
      & 1454.842 &  19.42  &     4.76  &    12.93   \\
      & 1709.600 &  21.14  &     5.50  &    12.79  \\
      & 1741.549 & 21.25  &     5.41  &    12.77  \\
      & 1751.910 & 21.35  &     5.17  &    12.94  \\
S II & 1250.584 & 21.28  &     5.50  &    14.39:  \\
   &  1253.811 & 22.24  &     3.38  &    14.17  \\
Si II & 1808.013 &  18.91  &     5.04  &    14.52 \\  
%       &  &  &  &  \\
Al III & 1854.716 & 20.00  &     7.00  &    11.79  \\ 
       & 1862.790 & 19.00  &     7.66  &    11.72  \\ 
C IV  & 1548.195 & 27.88  &    12.00  &    12.73  \\
     & 1550.770 & 27.42  &    10.61  &    12.56  \\ 
%      &  &  &  &  \\
%       &  &  &  &  \\
%        &  &  &  &  \\ 
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\multicolumn{5}{c}{35 km s$^{-1}$ Component}\\ 
\hline               
Al II & 1670.787$^{b}$ & 31.12  &     3.80  &    11.28  \\
      & 1670.787$^{a}$ & 29.51  &     2.19  &    11.08   \\
Fe II & 2382.765 & 36.00  &     1.50  &    11.40  \\
      & 2600.173 & 37.11  &     1.61  &    11.51   \\
Mg II & 2796.352 &  37.81  &     5.00  &    12.04 \\
      & 2803.531 & 37.23  &     5.00  &    12.09  \\
O I & 1302.169 & 38.09  &     4.44  &    13.40  \\
Si II & 1526.707 & 38.49  &     3.70  &    12.28  \\
%       &  &  &  &  \\
Al III & 1854.716 & 35.55  &     8.47  &    11.61  \\
\hline
\multicolumn{5}{c}{50 km s$^{-1}$ Component}\\
 \hline   
Al II & 1670.787$^{a}$ & 49.61  &     1.73  &    10.90   \\
      & 1670.787$^{b}$ &  50.00  &     2.00  &    10.95  \\
Fe II & 2382.765 & 49.42  &     1.74  &    12.18  \\
      & 2586.650 & 49.98  &     1.50  &    11.87:   \\
      & 2600.173 &   49.53  &     2.50  &    12.16  \\
Mg II & 2796.352 & 50.23  &     4.09  &    12.20  \\
      & 2803.531 &  50.08  &     4.73  &    12.23  \\
 O I & 1302.169 &  48.75  &     3.61  &    13.45  \\
Si II & 1526.707 & 48.96  &     3.02  &    12.33  \\
\hline
\multicolumn{5}{c}{61 km s$^{-1}$ Component}\\ 
\hline   
Al II & 1670.787$^{a}$ &  60.98  &     4.00  &    12.17: \\
      & 1670.787$^{b}$ &  60.42  &     4.95  &    12.21: \\
Fe II & 1608.451 & 60.08  &     3.00  &    12.87   \\
      & 2586.650 &  59.94  &     3.50  &    13.06  \\
Mg I & 2852.964 &  65.00  &     4.31  &    11.30   \\
Mn II & 2576.877 & 61.15  &     4.00  &    11.36  \\
S II & 1250.584 & 63.23  &     3.50  &    13.74  \\
     & 1253.811 & 62.74  &     3.50  &    13.59  \\
Si II & 1526.707 & 60.16  &     3.50  &    13.23:   \\
%       &  &  &  &  \\
Al III & 1854.716 & 56.96  &     5.97  &    11.45  \\
C IV & 1548.195 & 55.19  &    12.00  &    12.64  \\
    &  1550.770  & 57.60  &    12.00  &    12.64  \\
Si IV & 1393.755 & 58.50  &    12.00  &    11.65: \\
     & 1402.770 & 61.33  &     7.22  &    11.79  \\
\hline
\multicolumn{5}{c}{71 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & 71.00  &     4.07  &    13.68:   \\
      & 1670.787$^{b}$ & 71.00  &     5.73  &    13.30:  \\
Fe II & 1608.451 &  71.10  &     6.02  &    14.24:  \\
      &  1611.201 & 71.66  &     3.90  &    14.09 \\
      & 2586.650 & 70.92  &     5.20  &    14.35: \\
Mg I & 2852.964 &  72.55  &     2.68  &    11.90  \\
Mn II & 2576.877 &  71.75  &     6.36  &    12.31  \\
      & 2594.499 & 71.00  &     6.44  &    12.28  \\
      & 2606.462 &  70.59  &     6.03  &    12.28  \\
Ni II & 1317.217$^{c}$ & 72.00  &     5.95  &    12.92  \\
     & 1317.217$^{d}$ & 72.33  &     5.54  &    12.98  \\
       & 1370.132 &  72.34  &     7.66  &    13.06  \\
       & 1709.600 &  70.72  &     9.06  &    13.19  \\
       & 1741.549 & 71.60  &     6.15  &    13.11  \\
       & 1751.910 & 73.16  &     4.40  &    12.85  \\
O I* & 1304.858 & 70.89  &     5.20  &    12.76 \\
O I** & 1306.029 & 70.87  &     5.55  &    12.83  \\
S II & 1250.584 & 72.29  &     5.22  &    14.50  \\
    & 1253.811 & 72.14  &     5.36  &    14.46  \\
\\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline

Si II & 1526.707 &   71.00  &     7.37  &    14.36:  \\
      & 1808.013 &  71.13  &     5.61  &    14.56  \\
Si II* & 1264.738 & 72.22  &     4.02  &    12.50:  \\
       & 1265.002 & 72.00  &     3.05  &    12.36  \\
       & 1309.276 & 71.40  &     3.66  &    12.06  \\
%       &  &  &  &  \\
Al III & 1854.716 & 70.71  &     6.56  &    11.93 \\
       & 1862.790 & 71.07  &     9.24  &    11.94  \\
\hline
\multicolumn{5}{c}{83 km s$^{-1}$ Component}\\ 
\hline      
Al II & 1670.787$^{b}$ & 80.61  &     3.00  &    11.86: \\
      & 1670.787$^{a}$ & 80.77  &     3.00  &    12.13:   \\
Fe II & 1608.451 & 82.81  &     3.00  &    13.14:  \\
      & 2586.650 &  81.02  &     3.00  &    13.23:  \\
Mg I & 2852.964 & 78.50  &     4.00  &    11.20  \\
S II & 1250.584 & 83.08  &     2.17  &    13.55  \\
     & 1253.811 & 83.67  &     2.53  &    13.58  \\
Si II & 1526.707 & 82.54  &     2.50  &    13.22:   \\
%       &  &  &  &  \\
C IV & 1548.195 & 78.33  &    12.00  &    12.63  \\
     & 1550.770 & 75.54  &    12.00  &    12.59  \\ 
Si IV & 1393.755 & 81.68  &    11.64  &    11.97  \\
       & 1402.770 & 82.36  &     9.41  &    12.03  \\         
\hline
\multicolumn{5}{c}{90 km s$^{-1}$ Component}\\ 
\hline             
Al II & 1670.787$^{a}$ & 90.00  &     5.59  &    12.81:   \\
      & 1670.787$^{b}$ & 90.00  &     5.93  &    13.03:  \\
Fe II & 1608.451 &  90.03  &     4.22  &    13.84  \\
      & 2586.650 &  90.29  &     5.03  &    13.93  \\
Mg I & 2852.964 &  90.09  &     5.20  &    11.62   \\
Mg II & 1240.395 & 92.30  &     1.50  &    14.37:  \\
Mn II & 2576.877 &  89.75  &     5.32  &    11.99  \\
      & 2594.499 & 90.36  &     5.50  &    11.90  \\
      & 2606.462 &  89.00  &     5.55  &    11.99 \\
Ni II  & 1317.217$^{d}$ & 91.67  &     8.67  &    12.82  \\
      & 1370.132 & 91.52  &     4.61  &    12.53  \\
      & 1709.600 & 92.43  &     8.51  &    12.91  \\
      & 1741.549 & 91.78  &     8.20  &    12.90  \\
      & 1751.910 & 90.62  &     5.28  &    12.66  \\
O I* & 1304.858 &  90.54  &     4.65  &    12.65  \\
O I** & 1306.029 & 93.01  &     7.56  &    12.70  \\
S II & 1250.584 & 91.01  &     4.72  &    14.29  \\
     & 1253.811 & 90.64  &     3.59  &    14.24  \\
Si II & 1526.707 & 90.00  &     6.89  &    14.08:   \\
      & 1808.013 & 91.02  &     4.81  &    14.35  \\
Si II* & 1264.738 & 90.73  &     4.21  &    12.14  \\
       & 1265.002 &  92.51  &     1.95  &    11.87:  \\
%       &  &  &  &  \\
Al III & 1854.716 & 89.28  &     9.97  &    11.93  \\
      & 1862.790 & 92.83  &    10.99  &    11.82  \\
\hline
\multicolumn{5}{c}{98 km s$^{-1}$ Component}\\ 
\hline       
Al II & 1670.787$^{a}$ & 98.00  &     4.00  &    12.30:  \\
      & 1670.787$^{b}$ & 98.00  &     4.19  &    12.01:  \\
Fe II & 1608.451 & 97.16  &     4.00  &    13.40  \\
      & 2586.650 & 98.27  &     3.60  &    13.29  \\
Mg I & 2852.964 &  98.60  &     3.40  &    11.11   \\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 4. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Mn II & 2576.877 & 98.50  &     4.71  &    11.53   \\
      & 2606.462 & 98.77  &     1.54  &    11.26:   \\
S II & 1250.584 & 98.88  &     3.50  &    13.81  \\
     & 1253.811 & 98.26  &     3.49  &    13.89  \\
Si II & 1526.707 & 98.00  &     3.60  &    14.04: \\
      & 1808.013 & 99.53  &     1.50  &    13.76:   \\
\hline
\multicolumn{5}{l}{$^a$ Exposure with central $\lambda$ = 1598 \AA}\\
\multicolumn{5}{l}{$^b$ Exposure with central $\lambda$ = 1763 \AA}\\
\multicolumn{5}{l}{$^c$ Exposure with central $\lambda$ = 1234 \AA}\\
\multicolumn{5}{l}{$^d$ Exposure with central $\lambda$ = 1416 \AA}\\
\multicolumn{5}{l}{Notes---Units for velocity v, dispersion b, and}\\ 
\multicolumn{5}{l}{column density N are, respectively, km~s$^{-1}$,}\\ 
\multicolumn{5}{l}{km~s$^{-1}$, and cm$^{-2}$. Column densities that}\\
\multicolumn{5}{l}{are more uncertain because of weak, blended,}\\ 
\multicolumn{5}{l}{or saturated components are marked with }\\ 
\multicolumn{5}{l}{colons. Error estimates are provided in the}\\
\multicolumn{5}{l}{text.}\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
\\
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\\
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\\
\\
\end{tabular}
}


%\documentclass[10pt]{paastex}
%\usepackage{myemulateapj5}
%\pagestyle{empty}
%\begin{document}
\clearpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. HD 93222}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
\multicolumn{5}{c}{$-$388 km s$^{-1}$ Component}\\ 
\hline
C II & 1334.532 & $-$388.00   &     5.86   &    12.99 \\
Mg II & 2796.352 & $-$388.21   &     6.46   &    11.54 \\
     & 2803.531 & $-$388.43   &     2.75   &    11.26  \\
\hline 
\multicolumn{5}{c}{$-$379 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$381.69   &     1.95   &    10.85 \\
      & 1670.787$^{b}$ & $-$378.17   &     6.00   &    11.08  \\
C II & 1334.532 &  $-$379.00   &     3.68   &    13.19 \\
Fe II & 2382.765 &  $-$379.62   &     1.50   &    11.28 \\
      & 2586.650 & $-$379.58  &    5.00  &   12.14  \\
      & 2600.173 & $-$378.83   &     2.31   &    11.58  \\
Mg II & 2796.352 & $-$379.00   &     3.43   &    11.77 \\
      & 2803.531 & $-$379.00   &     3.03   &    11.75 \\
Si II & 1304.370 & $-$379.00   &     5.53   &    12.23  \\
      & 1526.707 & $-$379.28   &     2.06   &    11.85  \\
\hline 
\multicolumn{5}{c}{$-$372 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$371.18   &     3.55   &    11.82 \\
      & 1670.787$^{b}$ & $-$372.40   &     2.98   &    11.67 \\
C II & 1334.532 & $-$372.00   &     3.54   &    13.86:  \\
Fe II & 1608.451 & $-$371.42  &    2.46  &   12.65 \\
      & 2382.765 & $-$372.28   &     1.65   &    12.47  \\
      & 2586.650 & $-$371.61  &    2.31  &   12.69 \\
      & 2600.173 & $-$371.90   &     1.76   &    12.53 \\
Mg I & 2852.964 & $-$370.21  &    3.36  &   10.70 \\
Mg II & 2796.352 & $-$371.08   &     3.04   &    12.74 \\
      & 2803.531 & $-$371.19   &     3.02   &    12.80 \\
O I & 1302.169  &  $-$370.73   &     3.65   &    13.31 \\
S II & 1253.811 & $-$372.00  &    1.50  &   12.86:  \\
Si II & 1304.370 & $-$370.88   &     3.18   &    13.02 \\
      & 1526.707 & $-$371.10   &     3.00   &    13.00 \\
Si II* & 1264.738 & $-$373.35  &     1.54  &    11.18  \\
%       &     &     &     &     \\
C IV & 1548.195 & $-$369.45  &     6.23  &    12.01  \\
%   &     &     &     &     \\
%   &     &     &     &     \\
%   &     &     &     &     \\
\hline 
\multicolumn{5}{c}{$-$365 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$363.99   &     4.55   &    11.51 \\
      & 1670.787$^{b}$ & $-$365.84   &     3.91   &    11.57 \\
C II & 1334.532 & $-$365.00   &     6.64   &    14.09:  \\
Fe II & 1608.451 & $-$364.13  &    1.50  &   12.16: \\
      & 2382.765 & $-$367.37   &     7.64   &    12.66  \\
      & 2586.650 & $-$365.01  &    2.66  &   12.34 \\
      & 2600.173 & $-$366.11   &     7.28   &    12.60 \\
Mg I & 2852.964 & $-$363.24  &    4.00  &   10.48 \\
Mg II & 2796.352 & $-$364.77   &     3.51   &    12.43 \\
      & 2803.531 & $-$365.55   &     2.38   &    12.12 \\
O I & 1302.169  &  $-$363.91   &     4.67   &    13.09 \\
S II & 1253.811 & $-$365.00  &    4.74  &   13.14:  \\
Si II & 1304.370 &  $-$365.00   &     2.81   &    12.49 \\
      & 1526.707 & $-$364.80   &     1.84   &    12.42 \\
\hline 
\multicolumn{5}{c}{$-$359 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$358.60   &     2.93   &    11.41 \\
      & 1670.787$^{b}$ & $-$359.84   &     2.40   &    11.38 \\
C II & 1334.532 & $-$359.00   &     5.05   &    13.67:  \\
Fe II & 1608.451 & $-$358.37  &    1.50  &   12.14: \\
      & 2382.765 &  $-$358.42   &     1.66   &    11.99  \\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
      & 2586.650 & $-$359.00  &    3.71  &   12.27 \\
      & 2600.173 & $-$358.40   &     1.50   &    11.92 \\
Mg I & 2852.964 & $-$357.14  &    1.50  &   10.48 \\
Mg II & 2796.352 & $-$358.15   &     3.23   &    12.33 \\
      & 2803.531 & $-$359.82   &     5.71   &    12.59 \\
O I & 1302.169  & $-$357.36   &     3.32   &    12.99 \\
Si II & 1304.370 & $-$359.00   &     5.01   &    12.81 \\
      & 1526.707 & $-$358.94   &     3.37   &    12.59 \\ 
%       &     &     &     &     \\
C IV & 1548.195 & $-$359.07  &     3.10  &    12.01 \\
    & 1550.770 &  $-$362.02  &     4.00  &    11.91  \\
Si IV & 1393.755 & $-$360.38  &     5.00  &    11.23:  \\
     & 1402.770 & $-$356.11  &     5.96  &    11.59:  \\
\hline 
\multicolumn{5}{c}{$-$350 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$350.65   &     4.45   &    10.70 \\
      & 1670.787$^{b}$ & $-$352.42   &     6.07   &    11.20 \\
C II & 1334.532 & $-$350.00   &     6.95   &    13.20 \\
Mg II & 2796.352 & $-$349.99   &     5.97   &    11.79 \\
      & 2803.531 & $-$346.19   &     4.00   &    11.56 \\  
%       &     &     &     &     \\ 
C IV & 1548.195 & $-$350.00  &     8.00  &    12.32  \\
\hline 
\multicolumn{5}{c}{$-$115 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$115.18   &     1.50   &    10.70 \\
      & 1670.787$^{b}$ & $-$114.71   &     2.86   &    11.11  \\
C II* & 1335.708 & $-$115.00   &     3.89   &    12.82  \\
Fe II  & 2382.765 & $-$115.50   &     1.50   &    11.40  \\
      & 2600.173 &  $-$115.99   &     2.37   &    11.72 \\
Mg II & 2796.352 & $-$115.09   &     2.92   &    11.74  \\
      & 2803.531 & $-$115.04   &     1.95   &    11.49 \\
O I & 1302.169 & $-$114.20   &     4.24   &    12.76:  \\
Si II & 1304.370 & $-$113.69   &     4.17   &    12.24:  \\
      & 1526.707 & $-$113.31   &     4.47   &    12.18 \\
%       &     &     &     &     \\
C IV & 1548.195 &   $-$124.00  &     3.25  &    11.69 \\
\hline 
\multicolumn{5}{c}{$-$110 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$109.61   &     2.86   &    11.32 \\
      & 1670.787$^{b}$ & $-$109.62   &     1.88   &    11.04  \\
C II* & 1335.708 & $-$110.00   &     3.56   &    12.23  \\
Fe II  & 2382.765 & $-$109.25   &     4.57   &    11.75  \\
      & 2600.173 & $-$110.01   &     1.50   &    11.51 \\
Mg II & 2796.352 & $-$109.88   &     3.24   &    11.95  \\
      & 2803.531 & $-$110.17   &     4.12   &    11.98 \\
Si II  & 1526.707 & $-$107.85   &     1.50   &    11.73 \\  
%       &     &     &     &     \\
Al III & 1854.716 & $-$108.34  &     2.58  &    10.95 \\
C IV & 1548.195 &  $-$106.00  &    11.11  &    12.76 \\
    & 1550.770 & $-$105.58  &     8.48  &    12.48  \\
Si IV & 1402.770 & $-$106.00  &     7.91  &    11.80 \\
\hline 
\multicolumn{5}{c}{$-$98 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$98.91   &     1.50   &    10.78: \\
C II* & 1335.708 & $-$97.00   &     4.03   &    12.67  \\
Mg II & 2796.352 & $-$98.20   &     4.14   &    11.89 \\
      & 2803.531 & $-$97.74   &     4.21   &    11.92 \\
Si II  & 1526.707 & $-$98.15   &     2.36   &    11.97 \\   
\hline 
\multicolumn{5}{c}{$-$87 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$86.09   &     5.13   &    11.82  \\
      & 1670.787$^{b}$ & $-$87.80   &     3.86   &    11.64 \\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
C II* & 1335.708 & $-$87.00   &     4.03   &    13.23  \\
Fe II  & 2382.765 & $-$88.13   &     3.60   &    12.05 \\
      & 2600.173 &  $-$87.80   &     3.05   &    12.05  \\
Mg I & 2852.964 & $-$87.00  &    3.39  &   10.60  \\
Mg II & 2796.352 & $-$87.24   &     3.89   &    12.61  \\
      & 2803.531 & $-$86.82   &     3.87   &    12.62 \\
S II & 1250.584 & $-$87.44  &    7.00  &   13.72:  \\
Si II & 1304.370 & $-$87.00   &     3.33   &    12.48 \\
      & 1526.707 & $-$87.54   &     3.03   &    12.64  \\
\hline 
\multicolumn{5}{c}{$-$81 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$80.27   &     2.34   &    11.20  \\
      & 1670.787$^{b}$ & $-$81.75   &     4.05   &    11.63 \\
C II* & 1335.708 &  $-$81.00   &     4.50   &    12.91: \\
Fe II  & 2382.765 & $-$82.15   &     2.85   &    11.93 \\
      & 2600.173 &  $-$81.75   &     2.28   &    11.89 \\
Mg I & 2852.964 & $-$81.00  &    3.50  &   10.60 \\
Mg II & 2796.352 & $-$81.41   &     3.18   &    12.22:  \\
      & 2803.531 & $-$80.71   &     3.73   &    12.47 \\
Si II & 1304.370 & $-$81.00   &     4.94   &    12.61 \\
      & 1526.707 & $-$81.14   &     4.66   &    12.74  \\
      & 1808.013 & $-$82.82   &     1.79   &    13.37:  \\  
%       &     &     &     &     \\
Al III & 1854.716 & $-$83.00  &     6.09  &    11.28  \\
C IV & 1548.195 & $-$83.09  &     9.27  &    13.59  \\
    & 1550.770 &  $-$83.29  &     7.87  &    13.54 \\
Si IV & 1402.770 & $-$82.73  &     9.88  &    13.00 \\
\hline 
\multicolumn{5}{c}{$-$68 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$66.82   &     7.77   &    12.54  \\
      & 1670.787$^{b}$ & $-$67.14   &     7.71   &    12.55 \\
Fe II & 1608.451 & $-$67.48  &    3.39  &   13.02 \\
      & 2382.765 &  $-$68.84   &     4.88   &    13.18 \\
      & 2586.650 &   $-$69.32  &    3.89  &   13.03 \\
      & 2600.173 &  $-$67.06   &     5.85   &    13.31  \\
Mg I & 2852.964 & $-$68.00  &    4.00  &   10.60  \\
S II & 1253.811 & $-$70.56  &    4.00  &   13.37  \\
     & 1259.519  & $-$68.18  &    5.42  &   13.12  \\
Si II & 1304.370 & $-$68.69   &     4.86   &    13.38 \\
      & 1526.707 & $-$70.81   &     3.84   &    13.17  \\
%       &     &     &     &     \\
Al III & 1854.716 &  $-$67.83  &     5.54  &    11.96 \\
       & 1862.790 & $-$67.82  &     5.84  &    11.69 \\   
C IV & 1548.195 &  $-$65.62  &     7.65  &    13.82  \\
    & 1550.770 & $-$65.79  &     7.61  &    13.83  \\
Si IV & 1393.755 & $-$66.10  &     7.69  &    13.34  \\
     & 1402.770 & $-$65.99  &     6.22  &    13.31 \\
\hline 
\multicolumn{5}{c}{$-$64 km s$^{-1}$ Component}\\ 
\hline
Al II & 1670.787$^{a}$ & $-$63.54   &     2.38   &    11.83 \\
      & 1670.787$^{b}$ & $-$64.41   &     1.50   &    11.79 \\
Fe II & 1608.451 & $-$63.13  &    1.50  &   12.73   \\
      & 2382.765 & $-$64.11   &     2.43   &    12.83   \\
      & 2586.650 &  $-$64.00  &    3.03  &   13.07  \\
      & 2600.173 & $-$64.00   &     1.50   &    12.59   \\
Mg I & 2852.964 & $-$64.66  &    4.11  &   11.53   \\
Mn II & 2576.877 & $-$64.38  &    6.06  &   11.53: \\
      & 2594.499 & $-$64.85  &    7.25  &   11.63: \\
      & 2606.462 & $-$63.47  &    4.00  &   11.51:  \\
\\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
S II & 1250.584 & $-$62.27  &    7.20  &   13.96:   \\
     & 1253.811 & $-$62.89  &    2.96  &   13.74  \\
     & 1259.519 & $-$63.56  &    2.55  &   13.49 \\
Si II & 1304.370 & $-$63.60   &     3.01   &    13.69 \\
      & 1526.707 &  $-$63.98   &     3.80   &    13.80  \\
     & 1808.013 & $-$65.49   &     4.56   &    13.87:  \\
Si II* & 1264.738 & $-$64.30  &     3.18  &    11.92  \\
\hline 
\multicolumn{5}{c}{$-$50 km s$^{-1}$ Component}\\ 
\hline
Fe II & 1608.451 & $-$50.07  &    3.22  &   13.28   \\
      & 2586.650 & $-$48.50  &    6.22  &   13.63 \\
      & 2600.173 &  $-$47.87   &     6.51   &    13.63:  \\
Mg I & 2852.964 & $-$52.44  &    3.49  &   11.53  \\
Mn II & 2576.877 & $-$50.00  &    3.81  &   11.30  \\
      & 2594.499 & $-$50.00  &    4.03  &   11.72 \\
      & 2606.462 & $-$50.00  &    4.00  &   11.28:  \\
Ni II & 1317.217$^{c}$ & $-$47.51  &    6.00  &   12.39: \\
S II & 1250.584 & $-$49.41  &    5.03  &   14.41  \\
     & 1253.811 & $-$50.61  &    5.37  &   14.40 \\
     & 1259.519 & $-$51.07  &    4.63  &   14.26  \\
Si II & 1808.013 & $-$48.78   &     5.70   &    14.54  \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$48.99  &     5.07  &    12.46  \\
       & 1862.790 & $-$48.70  &     4.86  &    12.38 \\   
C IV & 1548.195 & $-$46.71  &     8.00  &    13.50  \\
    & 1550.770 &  $-$46.90  &     7.76  &    13.44  \\
Si IV & 1393.755 & $-$48.55  &     5.18  &    12.83  \\
     & 1402.770 & $-$46.78  &     7.79  &    13.21 \\
\hline 
\multicolumn{5}{c}{$-$44 km s$^{-1}$ Component}\\ 
\hline
Fe II & 1608.451 & $-$43.93  &    2.38  &   13.40  \\
      & 2586.650 & $-$43.88  &    1.50  &   13.17 \\
      & 2600.173 & $-$44.00   &     5.71   &    13.65:  \\
Mg I & 2852.964 & $-$43.10  &    8.00  &   12.08: \\
Mn II & 2576.877 & $-$44.00  &    4.00  &   11.54: \\
      & 2594.499 & $-$44.00  &    3.52  &   11.54 \\
      & 2606.462 & $-$44.00  &    5.00  &   11.67:  \\
S II & 1250.584 & $-$43.36  &    1.62  &   13.77  \\
     & 1253.811 & $-$44.35  &    1.50  &   13.48 \\
     & 1259.519 & $-$44.42  &    2.41  &   13.75  \\
Si II & 1808.013 & $-$42.07   &     2.33   &    13.72  \\
Si II* & 1264.738 & $-$44.20  &     6.67  &    11.99:  \\
\hline 
\multicolumn{5}{c}{$-$38 km s$^{-1}$ Component}\\ 
\hline
Fe II & 1608.451 & $-$38.14  &    2.92  &   13.12  \\
      & 2586.650 & $-$38.36  &    3.74  &   13.29 \\
      & 2600.173 & $-$38.00   &     4.50   &    12.85:  \\
Mn II & 2594.499 & $-$38.00  &    4.00  &   11.64 \\
Ni II & 1317.217$^{c}$ & $-$36.36  &    5.00  &   12.15:   \\
S II & 1250.584 & $-$38.39  &    3.87  &   14.19  \\
     & 1253.811 & $-$37.73  &    7.57  &   14.52 \\
     & 1259.519 & $-$39.27  &    6.50  &   14.29  \\
Si II & 1808.013 & $-$37.90   &     2.88   &    13.91  \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$34.00  &     8.68  &    12.72  \\
       & 1862.790 & $-$34.00  &     8.11  &    12.68 \\   
C IV & 1548.195 & $-$33.79  &     5.45  &    13.55  \\
    & 1550.770 &  $-$33.97  &     5.57  &    13.54 \\
Si IV & 1393.755 & $-$33.60  &    10.69  &    13.64:  \\
     & 1402.770 & $-$34.50  &     6.43  &    13.45 \\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline 
\multicolumn{5}{c}{$-$23 km s$^{-1}$ Component}\\ 
\hline
B II & 1362.461 & $-$23.48   &     4.99   &    11.62 \\
Cl I & 1347.240 & $-$22.57   &     2.12   &    11.53  \\
Cu II & 1358.773 & $-$22.40   &     3.42   &    12.42  \\
Fe II & 1608.451 & $-$23.55  &    4.22  &   15.26: \\
      & 1611.201 & $-$23.07   &     3.04   &    15.00  \\
      & 2586.650 & $-$24.11  &    4.09  &   15.42: \\
Ga II & 1414.402 & $-$22.39   &     4.79   &    11.64  \\
Ge II & 1237.059 & $-$23.09   &     4.45   &    12.21  \\
Mg I & 2852.964 &  $-$24.60  &    3.91  &   13.80: \\
Mg II & 1239.925 & $-$23.29   &     4.93   &    16.00  \\
     & 1240.395 & $-$23.31   &     5.07   &    16.07  \\
Mn II & 2576.877 & $-$23.54  &    5.11  &   13.77:  \\
      & 2594.499 & $-$23.67  &    4.90  &   13.83:  \\
      & 2606.462 &  $-$23.72  &    5.10  &   13.78:  \\
Ni II & 1317.217$^{c}$ & $-$21.40  &    3.13  &   13.37  \\
      & 1317.217$^{d}$ & $-$22.03   &     3.14   &    13.37  \\
      & 1370.132 & $-$21.42  &    3.28  &   13.40  \\
      & 1709.600 & $-$21.29  &    2.76  &   13.50  \\
      & 1741.549 & $-$21.34  &    3.30  &   13.50  \\
      & 1751.910 & $-$20.59  &    2.33  &   13.42  \\
O I] & 1355.598 & $-$22.30   &     3.62   &    17.80  \\
O I* & 1304.858 & $-$23.69   &    4.35    &  14.32:  \\
O I** & 1306.029 & $-$24.87  &     4.52  &    14.13  \\
P II & 1532.533 & $-$23.48   &     4.33   &    14.23  \\
S I & 1425.030 & $-$23.10   &     2.32   &    11.72  \\
S II & 1250.584 & $-$23.56  &    4.83  &   16.17:  \\
     & 1253.811 & $-$23.97  &    3.86  &   16.70:  \\
Si II & 1808.013 & $-$23.89   &     4.67   &    16.36: \\
Si II* & 1264.738 & $-$24.94  &     5.31  &    14.19:  \\
       & 1265.002 & $-$24.87  &     5.06  &    14.28  \\
       & 1309.276 &  $-$24.92  &     5.26  &    13.99  \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$21.81  &     5.41  &    13.51: \\
       & 1862.790 & $-$21.28  &     5.25  &    13.55 \\   
C IV & 1548.195 & $-$19.80  &     6.91  &    13.72  \\
    & 1550.770 &  $-$19.76  &     6.65  &    13.68 \\
Si IV & 1393.755 & $-$17.76  &     3.56  &    14.95: \\
     & 1402.770 & $-$19.21  &     4.55  &    14.38 \\
\hline 
\multicolumn{5}{c}{$-$6 km s$^{-1}$ Component}\\ 
\hline
B II & 1362.461 & $-$6.70   &     1.65   &    11.08 \\
Cl I & 1347.240 & $-$7.12   &     1.91   &    13.23 \\
Cu II & 1358.773 & $-$5.80   &     2.53   &    12.05  \\
Fe II & 1608.451 & $-$6.00  &    4.74  &   14.74: \\
      & 1611.201 &  $-$5.85   &     3.20   &    14.84 \\
Ga II & 1414.402 & $-$6.34   &     3.77   &    11.30  \\
Ge II & 1237.059 & $-$6.35   &     3.35   &    11.96  \\
Mg I & 2852.964 &   $-$6.00  &    6.37  &   12.81: \\
Mg II & 1239.925 & $-$5.91   &     3.16   &    15.85  \\
     & 1240.395 & $-$5.86   &     3.19   &    15.90 \\
Mn II & 2576.877 & $-$6.45  &    3.24  &   13.69:  \\
      & 2594.499 & $-$6.54  &    3.58  &   13.55  \\
      & 2606.462 &  $-$6.76  &    3.85  &   13.43 \\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
Ni II & 1317.217$^{c}$ & $-$4.44  &    4.36  &   13.53  \\
      & 1317.217$^{d}$ & $-$5.04   &     3.97   &    13.53  \\
      & 1370.132 & $-$4.55  &    4.21  &   13.51  \\
      & 1709.600 & $-$3.84  &    4.05  &   13.61  \\
      & 1741.549 & $-$4.34  &    4.58  &   13.67 \\
      & 1751.910 & $-$3.64  &    3.61  &   13.56 \\
\mbox{O I]} & 1355.598 & $-$6.88   &     2.85   &    17.50  \\
P II & 1532.533 &  $-$6.49   &     3.45   &    14.03  \\
S I & 1425.030 & $-$7.18   &     2.84   &    12.18  \\
S II & 1250.584 & $-$6.00  &    4.88  &   15.64: \\
     & 1253.811 & $-$6.00  &    5.04  &   15.89:  \\
Si II & 1808.013 &  $-$5.21   &     4.86   &    15.73: \\
%       &     &     &     &     \\
Al III & 1854.716 & $-$5.82  &     4.10  &    12.03 \\
       & 1862.790 & $-$4.89  &     4.07  &    12.08 \\   
C IV & 1548.195 & $-$7.00  &     8.00  &    13.22  \\
    & 1550.770 &  $-$7.00  &     9.00  &    13.20 \\
Si IV & 1393.755 & $-$5.72  &     5.40  &    12.76 \\
     & 1402.770 & $-$7.27  &     8.00  &    12.99 \\
%       &     &     &     &     \\
\hline 
\multicolumn{5}{c}{6 km s$^{-1}$ Component}\\ 
\hline
B II & 1362.461 & 6.16   &     7.24   &    11.36  \\
Cl I & 1347.240 & 4.61   &     1.97   &    13.68 \\
Cu II & 1358.773 & 6.26   &     4.27   &    12.07  \\
Fe II & 1608.451 &  6.00  &    6.20  &   14.86: \\
      & 1611.201 & 5.80   &     6.19   &    14.99 \\
Ga II & 1414.402 &  6.24   &     3.74   &    11.28 \\
Ge II & 1237.059 &  6.46   &     3.92   &    12.08  \\
Mg I & 2852.964 &   6.00  &    7.00  &   12.88: \\
Mg II & 1239.925 & 6.78   &     5.42   &    15.86  \\
     & 1240.395 & 6.78   &     4.75   &    15.88 \\
Mn II & 2576.877 & 6.00  &    4.76  &   13.63:  \\
      & 2594.499 & 5.89  &    5.00  &   13.57:  \\
      & 2606.462 &   5.49  &    5.73  &   13.51 \\
Ni II & 1317.217$^{c}$ & 7.34  &    6.20  &   13.63 \\
      & 1317.217$^{d}$ & 6.73   &     6.26   &    13.63 \\
      & 1370.132 & 7.44  &    6.73  &   13.67 \\
     & 1709.600 &  7.91  &    6.12  &   13.74  \\
      & 1741.549 & 7.48  &    6.17  &   13.76 \\
      & 1751.910 &  7.95  &    6.46  &   13.75 \\
\mbox{O I]} & 1355.598 & 6.25   &     6.28   &    17.71  \\
P II & 1532.533 &   5.99   &     4.91   &    14.14  \\
S I & 1425.030 &  5.59   &     1.94   &    12.45 \\
S II & 1250.584 & 6.00  &    8.67  &   15.91: \\
     & 1253.811 & 6.00  &    7.07  &   16.18: \\
Si II & 1808.013 &  7.32   &     4.27   &    15.98: \\
Si II* & 1264.738 & 10.02  &     3.12  &    11.08  \\
%       &     &     &     &     \\
Al III & 1854.716 & 5.63  &     8.67  &    12.79 \\
       & 1862.790 &  6.24  &     8.58  &    12.80 \\   
C IV & 1548.195 & 5.15  &     8.00  &    13.18  \\
    & 1550.770 &  6.00  &     9.44  &    13.19 \\
Si IV & 1393.755 & 4.72  &     5.58  &    12.82 \\
     & 1402.770 & 5.00  &     7.00  &    12.87 \\
\\
\end{tabular}
}
\newpage
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. \emph{Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline 
\multicolumn{5}{c}{17 km s$^{-1}$ Component}\\ 
\hline      
Fe II  & 1608.451 & 17.00  &    3.50  &   13.85: \\
Mg I & 2852.964 & 17.00  &    2.25  &   11.74  \\
Mg II & 1240.395 & 16.97   &     1.50   &    14.35:  \\
Mn II & 2576.877 & 17.00  &    4.00  &   12.04  \\
      & 2594.499 &  17.00  &    4.00  &   12.10  \\
      & 2606.462 & 17.00  &    4.00  &   11.86  \\
Si II & 1808.013 & 17.00   &     2.71   &    14.48  \\
%       &     &     &     &     \\
Al III & 1854.716 & 17.00  &     3.23  &    11.11 \\
       & 1862.790 &  17.00  &     1.50  &    11.11 \\   
C IV & 1548.195 &  17.00  &     9.00  &    12.82 \\
    & 1550.770 & 17.00  &     7.00  &    12.74  \\
Si IV & 1393.755 & 16.74  &     5.48  &    12.88 \\
     & 1402.770 &  16.62  &     6.42  &    12.92 \\
\hline 
\multicolumn{5}{c}{23 km s$^{-1}$ Component}\\ 
\hline  
Cl I & 1347.240 & 22.45   &     6.28   &    11.95  \\
Fe II & 1608.451 &  23.37  &    2.91  &   13.79  \\
      & 1611.201 & 22.97   &     1.50   &    13.74  \\
Mg I & 2852.964 & 22.85  &    2.02  &   12.01  \\
Mn II & 2576.877 & 23.00  &    4.22  &   11.92   \\
      & 2594.499 & 23.00  &    4.12  &   12.00  \\
      & 2606.462 & 23.00  &    3.72  &   11.90 \\
Ni II & 1317.217$^{c}$ & 21.98  &    4.34  &   12.74  \\
      & 1317.217$^{d}$ & 21.81   &     4.03   &    12.51  \\
       & 1370.132 & 22.78  &    5.00  &   12.89 \\
      & 1741.549 & 22.39  &    7.25  &   13.08  \\
      & 1751.910 & 22.54  &    3.29  &   12.51  \\
S II & 1250.584 & 24.14  &    2.16  &   14.07 \\
     & 1253.811 &  23.00   &    3.50   &   14.38 \\
     & 1259.519 & 23.41  &    2.04  &   14.07  \\
Si II  & 1808.013 & 23.00   &     2.69   &    14.29 \\ 
%       &     &     &     &     \\
C IV & 1548.195 &  25.00  &    12.00  &    12.97 \\
    & 1550.770 &  25.00  &     6.00  &    12.58 \\
Si IV & 1393.755 & 25.00  &     5.50  &    12.31 \\
     & 1402.770 &  27.64  &     7.00  &    12.31 \\
\hline 
\multicolumn{5}{c}{43 km s$^{-1}$ Component}\\ 
\hline  
Al II & 1670.787$^{b}$ &  42.62   &     2.89   &    10.70 \\
Mg II & 2796.352 & 41.77   &     6.88   &    11.34  \\
      & 2803.531 & 43.06   &     1.50   &    11.18:  \\
O I & 1302.169 & 40.63   &     6.75   &    12.80  \\
S II & 1253.811 &  43.00   &   7.13   &  13.75: \\
       &     &     &     &     \\
C IV & 1548.195 &  46.78  &    12.00  &    12.46 \\
Si IV & 1393.755 & 52.19  &     6.12  &    11.94 \\
     & 1402.770 & 49.52  &     6.97  &    12.16 \\
\hline
\multicolumn{5}{c}{65 km s$^{-1}$ Component}\\ 
\hline  
Al II & 1670.787$^{a}$ & 64.12   &     7.38   &    11.15 \\
      & 1670.787$^{b}$ & 66.31   &     2.33   &    10.70 \\
C II & 1334.532 & 65.00   &     3.19   &    13.00: \\
C II* & 1335.708 & 65.00   &     4.06   &    13.01 \\
Fe II & 2382.765 &  64.30   &     1.85   &    11.96 \\
      & 2600.173  & 64.49   &     2.34   &    11.94  \\
Mg II & 2796.352 & 64.50   &     2.17   &    11.83 \\
      & 2803.531 & 64.50   &     2.65   &    11.92  \\
\end{tabular}
\hspace{.4in}\hbox{
\begin{tabular}{llrrl}
\multicolumn{5}{c}{Table 5. {\it Continued}}\\
\\
\hline
Ion &\multicolumn{1}{c}{$\lambda$} &\multicolumn{1}{c}{v} &\multicolumn{1}{c}{b} &Log N\\
\hline
O I & 1302.169 & 64.50   &     4.39   &    13.12  \\
S II & 1253.811 & 65.00  &    8.46  &   13.74: \\ 
Si II & 1304.370 & 65.00   &     1.50   &    12.07 \\
     & 1526.707 & 65.16   &     2.81   &    12.27  \\
%       &     &     &     &     \\
C IV & 1548.195 &  65.00  &     7.94  &    11.92 \\
Si IV & 1393.755 & 65.96  &     3.11  &    11.85 \\
     & 1402.770 & 64.67  &     2.14  &    11.79 \\
\hline 
\multicolumn{5}{c}{72 km s$^{-1}$ Component}\\ 
\hline 
Al II & 1670.787$^{a}$ & 72.29   &     2.51   &    11.62 \\
      & 1670.787$^{b}$ & 72.56   &     4.00   &    11.85 \\
C II & 1334.532 & 72.00   &     6.51   &    14.12: \\
C II* & 1335.708 & 71.50   &     3.61   &    13.37: \\ 
Fe II & 1608.451 & 72.79  &    3.63  &   12.92  \\
     & 2382.765 & 71.37   &     2.53   &    12.83  \\
     & 2586.650 & 72.03  &    2.41  &   12.85  \\
     & 2600.173 & 71.74   &     2.55   &    12.83  \\    
Mg II & 2796.352 &  71.50   &     3.20   &    12.77 \\
      & 2803.531 & 71.50   &     3.09   &    12.83  \\
Mn II & 2576.877 & 72.00  &    8.15  &   11.51: \\
O I & 1302.169 & 71.50   &     4.59   &    14.20  \\
S II & 1253.811 & 72.00  &    4.47  &   13.18:  \\
    & 1259.519 & 73.27  &    7.25  &   13.20:  \\
Si II & 1526.707 & 72.73   &     3.11   &    13.18  \\ 
Si II* & 1264.738 & 75.25  &     6.41  &    11.52  \\    
\hline 
\multicolumn{5}{c}{78 km s$^{-1}$ Component}\\ 
\hline 
Al II & 1670.787$^{a}$ & 77.71   &     4.02   &    11.68 \\
      & 1670.787$^{b}$ & 79.16   &     4.29   &    11.40 \\
C II & 1334.532 & 78.00   &     4.34   &    14.02: \\
C II* & 1335.708 & 77.50   &     5.15   &    13.73: \\ 
Fe II & 1608.451 & 78.00  &    6.08  &   12.79 \\
     & 2382.765 & 76.86   &     4.19   &    12.77 \\
     & 2586.650 & 78.00  &    3.56  &   12.67 \\
     & 2600.173 & 77.47   &     3.79   &    12.74 \\    
Mg II & 2796.352 &  77.50   &     4.22   &    12.79 \\
      & 2803.531 & 77.50   &     4.40   &    12.78  \\
O I & 1302.169 & 77.50   &     4.57   &    14.28  \\
S II & 1253.811 & 78.00  &    8.06  &   13.60:  \\
Si II & 1526.707 & 78.56   &     3.73   &    12.94  \\     
\hline 
\multicolumn{5}{c}{93 km s$^{-1}$ Component}\\ 
\hline 
Al II & 1670.787$^{b}$ & 93.06   &     2.38   &    10.48: \\
Fe II & 2382.765 & 92.21   &     1.93   &    11.40 \\
\hline
\multicolumn{5}{l}{$^a$ Exposure with central $\lambda$ = 1598 \AA}\\
\multicolumn{5}{l}{$^b$ Exposure with central $\lambda$ = 1763 \AA}\\
\multicolumn{5}{l}{$^c$ Exposure with central $\lambda$ = 1234 \AA}\\
\multicolumn{5}{l}{$^d$ Exposure with central $\lambda$ = 1416 \AA}\\
\multicolumn{5}{l}{Notes---Units for velocity v, dispersion b, and}\\ 
\multicolumn{5}{l}{column density N are, respectively, km~s$^{-1}$,}\\ 
\multicolumn{5}{l}{km~s$^{-1}$, and cm$^{-2}$. Column densities that}\\
\multicolumn{5}{l}{are more uncertain because of weak, blended,}\\ 
\multicolumn{5}{l}{or saturated components are marked with }\\ 
\multicolumn{5}{l}{colons. Error estimates are provided in the}\\
\multicolumn{5}{l}{text.}\\
\\
\\
\end{tabular}
}

%\documentclass[10pt,preprint]{paastex}
%\thispagestyle{empty}
%\begin{document}
\clearpage

\begin{deluxetable}{ccccccccccc}
\tablenum{6}
\tablecaption{Comparative List of Low- and High-Ionization Interstellar Velocity          
Components\break toward Four Stars in the Carina Nebula [km~s$^{-1}$]\break
~~~~}
\tablewidth{0pt}
\tablehead{
\multicolumn{2}{c}{CPD~$-59^{\circ}$~2603} &\colhead{} &\multicolumn{2}{c}{HD~93205} 
&\colhead{} &\multicolumn{2}{c}{HDE~303308} &\colhead{} &\multicolumn{2}{c}{HD~93222}\\
\cline{1-2} \cline{4-5} \cline{7-8} \cline{10-11} \\
\colhead{Low} &\colhead{High} &\colhead{} &\colhead{Low} &\colhead{High} &\colhead{} 
&\colhead{Low} &\colhead{High} &\colhead{} &\colhead{Low} &\colhead{High}  }
\startdata
$-$233      &\phs\nodata & &\phs\nodata &\phs\nodata & &\phs\nodata &\phs\nodata 
& &\phs\nodata &\phs\nodata\\ 
$-$216      &\phs\nodata & &\phs\nodata &\phs\nodata & &\phs\nodata &\phs\nodata 
& &\phs\nodata &\phs\nodata\\ 
$-$185      &\phs\nodata & &\phs\nodata &\phs\nodata & &\phs\nodata &\phs\nodata 
& &\phs\nodata &\phs\nodata\\
$-$166      &$-$170      & &\phs\nodata &\phs\nodata & &$-$175      &\phs\nodata 
& &\phs\nodata &\phs\nodata\\
$-$153      &$-$158      & &\phs\nodata &\phs\nodata & &\phs\nodata &\phs\nodata 
& &\phs\nodata &\phs\nodata\\ 
$-$137      &$-$128      & &$-$142      &$-$130      & &$-$133      &$-$133  
& &\phs\nodata &\phs\nodata\\ 
$-$120      &$-$113      & &\phs\nodata &\phs\nodata & &\phs\nodata &\phs\nodata 
& &$-$115  &$-$124\\
\phs\nodata &\phs\nodata & &\phs\nodata &\phs\nodata & &$-$111      &$-$110  
& &$-$110  &$-$106\\
$-$101      &\phn$-$98   & &\phn$-$98   &$-$100      & &$-$104      &\phs\nodata 
& &\phn$-$98   &\phs\nodata\\ 
\phs\nodata &\phn$-$86 & &$-$89/$-$83   &\phn$-$90   & &$-$91/$-$82 &\phn$-$93 
& &$-$87/$-$81 &\phn$-$83\\
\phn$-$77   &\phn\nodata & &\phn$-$75   &\phs\nodata & &$-$76/$-$71 &\phn$-$78  
& &\phs\nodata &\phs\nodata \\
\phn$-$63   &\phn$-$69   & &\phn$-$66   &\phn$-$61   & &\phn$-$61   &\phn$-$60   
& &$-$68/$-$64 &\phn$-$66\\
\phs\nodata &\phs\nodata & &$-$58/$-$53 &\phs\nodata & &\phn$-$54   &\phs\nodata 
& &\phn$-$50  &\phn$-$48\\
\phn$-$38   &\phn$-$44   & &\phn$-$35   &\phn$-$35   & &$-$41/$-$33 &\phn$-$33  
& &$-$44/$-$38 &\phn$-$34\\
\phn$-$28   &\phn$-$30   & &\phs\nodata &\phs\nodata & &\phn$-$24   &\phs\nodata 
& &\phn$-$23   &\phn$-$20\\
\phn$-$19   &\phn$-$19   & &\phn$-$18   &\phn$-$18   & &\phn$-$16   &\phn$-$15   
& &\phs\nodata &\phs\nodata\\ 
\phn\phn$-$3 &\phn\phn$-$6 & &\phn\phn$-$3 &\phn\phn$-$3 & &\phn\phn$-$3 &\phn\phn$-$3 
& &\phn\phn$-$6 &\phn\phn$-$6\\
\phn\phn\phs8 &\phn\phn\phs6 & &\phn\phn\phs8 &\phn\phn\phs8 & &\phn\phn\phs7 
&\phn\phn\phs6 & &\phn\phn\phs6 &\phn\phn\phs6\\
\phn\phs17  &\phn\phs16  & &\phn\phs18   &\phn\phs18  & &\phn\phs19 &\phs\nodata 
& &\phn\phs17 &\phn\phs17\\
\phn\phs26  &\phs\nodata & &\phn\phs27   &\phn\phs27  & &\phs\nodata &\phn\phs23      
& &\phn\phs23 &\phn\phs25\\
\phn\phs38  &\phn\phs33  & &\phn\phs35   &\phn\phs35  & &\phn\phs35 &\phn\phs35      
& &\phs\nodata &\phs\nodata\\
\phn\phs61  &\phn\phs66  & &\phs\nodata  &\phs\nodata & &\phn\phs61 &\phn\phs58      
& &\phn\phs65 &\phn\phs65\\
69/72       &\phs\nodata & &\phn\phs69   &\phs\nodata & &\phn\phs71 &\phn\phs71 
& &\phn\phs72 &\phs\nodata\\
\phs\nodata &\phs\nodata & &\phn\phs80   &\phn\phs82  & &\phn\phs83 &\phn\phs79      
& &\phn\phs78 &\phs\nodata\\
\phs\nodata &\phs\nodata & &\phn\phs88   &\phn\phs92  & &\phn\phs90 &\phn\phs91      
& &\phn\phs93 &\phs\nodata\\
\phn\phs98  &\phs\nodata & &\phs100      &\phs104     & &\phn\phs98 &\phs\nodata 
& &\phs\nodata &\phs\nodata\\ 
\phs110     &\phs\nodata & &108/113      &\phs\nodata & &\phs\nodata &\phs\nodata 
& &\phs\nodata &\phs\nodata\\    
\phs120     &\phs\nodata & &\phs118      &\phs118     & &\phs\nodata &\phs\nodata 
& &\phn\nodata &\phs\nodata\\
\phs127     &\phs\nodata & &\phs\nodata  &\phs\nodata & &\phs\nodata &\phs\nodata 
& &\phs\nodata &\phs\nodata\\     
\enddata
\end{deluxetable}

\end{document}
                 

