PMSU1 - Table 1C: Early-type stars, giants and degenerates

Positions, distances, absolute magnitudes and spectral types for misclassified pCNS3 stars north of declination -30o. Note that `early-type' in this context means earlier than spectral type M. These are stars which have spectral characteristics inconsistent with the absolute magnitude assigned in pCNS3. Many are from Wolley et al's (1970) extension of Gliese's CNS1.
The format is similar to Tables 1A and 1B, save that we list apparent magnitude in addition to the inferred absolute magnitude. Positions from the following sources:
1. Co-ordinates measured at the Palomar 60-inch telescope
2. Co-ordinates measured at either the Palomar 200-inch telescope, Keck or the AAT
3. HST Guide Star catalogue (version 1)
4. pCNS3
5. Digital Sky Survey images
6. Hipparcos
Distances are derived from a variety of sources, in some cases Hipparcos parallax data (note that stars at distances beyond 50 parsecs generally have associated uncertainties of >10%), but primarily from spectroscopic parallaxes.

Spectral type
NN Name RA (2000) Dec Ref V MV Dist (pc) Source Notes
176 GJ 1023 A 0: 54: 18.0 69: 2: 50 6 9.70 4.37 116.4 110 G0
177 GJ 1023 B 0: 54: 18.0 69: 2: 50 6 10.40 5.07 116.4 110 G0
183 G269-061 0: 56: 19.5 -28: 8: 21 3 10.96 6.73 70.0 0 K3
185 Gl 44 0: 57: 20.4 -1: 48: 56 6 9.46 6.06 47.9 110 K1
188 GJ 2017 0: 59: 51.7 -25: 35: 26 6 9.87 4.55 116.0 110 G0
192 GJ 2019 1: 0: 37.0 -26: 38: 15 6 10.11 5.27 92.7 110 G5
198 GJ 2020 1: 1: 49.3 -25: 53: 12 6 9.75 3.03 220.8 110 F2
201 RG 2913 1: 1: 54.2 -25: 45: 38 3 11.84 7.78 65.0 0 K5
228 Gl 53.3 1: 9: 43.8 35: 37: 15 6 2.05 -1.88 61.1 110 M0 III A
306 BD+63 219 1: 41: 9.9 63: 48: 43 3 10.07 3.85 175.0 0 A5
387 Rob 115 2: 10: 13.4 11: 31: 58 3 12.72 -0.77 5000.0 0 M4 III B
579 AC+0:641-15 3: 14: 20.3 0: 39: 11 3 9.40 6.68 35.0 0 G3 B
602 LP355-65B 3: 22: 52.7 27: 8: 44 2 18.00 15.61 30.0 0 DC C
666 Wo 9124 3: 44: 20.0 24: 47: 45 3 10.66 5.09 130.0 0 K1
667 Wo 9125 3: 44: 20.4 24: 46: 21 3 10.81 5.33 125.0 0 K5
669 Wo 9127 3: 44: 22.1 24: 45: 57 4 11.09 6.20 95.0 0 G0
720 Gl 160.2 4: 6: 34.8 -20: 51: 4 6 9.68 7.82 23.5 110 K4
755 Gl 168.1 4: 22: 10.3 19: 28: 59 3 15.04 6.77 450.0 0 G0 *
757 LH190 4: 22: 16.5 15: 30: 44 2 17.00 12.00 100.0 0 M1?* B
763 VA42 4: 25: 0.2 16: 59: 4 3 10.31 7.04 45.0 0 K3
820 AC19:151 4: 43: 26.5 19: 0: 18 3 13.40 6.50 240.0 0 G0 B
909 GJ 2040 5: 19: 34.9 3: 52: 26 6 9.86 -6.16 16000.0 110 K0
985 Gl 223.1 5: 54: 34.0 -9: 23: 37 6 10.71 7.79 38.3 110 K4
1306 V518 8: 18: 44.4 -15: 12: 8 6 9.84 7.18 34.1 110 K3
1314 Gl 305.1 8: 23: 30.7 21: 50: 59 6 9.54 7.38 27.0 110 K3
1354 GJ 1113 8: 40: 36.8 43: 6: 52 6 9.32 6.86 31.0 110 K2
1384 GJ 1115 8: 53: 47.4 35: 13: 22 6 9.30 7.23 25.9 110 K3
1418 GJ 1120 A 9: 1: 17.5 15: 15: 59 6 9.43 8.12 18.3 110 K4
1597 Gl 383.1 10: 13: 57.3 52: 30: 30 6 9.53 7.74 22.8 110 K2
1689 Gl 402.1 10: 52: 2.7 0: -9: 35 6 10.20 6.78 48.2 110 K0
1714 Gl 409 11: 1: 57.2 -17: 57: 23 3 11.87 4.75 265.0 0 G5
1785 LHS2404 B 11: 25: 18.2 78: 16: 58 3 12.65 8.76 60.0 0 K0
1885 Gl 454.1 12: 1: 7.3 -1: 43: 55 6 10.96 7.77 43.5 110 K3
1912 Wo 9394 12: 12: 1.5 13: 15: 44 6 10.18 4.99 109.2 110 F2
2034 Gl 489 12: 57: 44.2 -14: 27: 48 6 9.12 7.29 23.2 110 K3
2053 Gl 499.1 13: 6: 22.6 22: 36: 58 6 5.60 -0.62 175.4 110 M5 III E
2149 Gl 518.2B 13: 37: 13.9 30: 5: 13 6 10.51 7.09 48.3 110 K1
2197 GJ 1180 13: 51: 59.6 26: 38: 11 6 10.83 4.81 160.0 110 G5
2213 LT 5453 13: 59: 7.6 -23: 33: 28 4 14.93 14.72 11.0 0 DA F
2287 Gl 550.1 14: 27: 45.3 23: 50: 26 6 10.92 7.70 44.1 110 K4
2328 Gl 561 14: 43: 19.3 26: 44: 59 6 9.67 5.46 69.6 110 K0
2335 Gl 562 14: 46: 23.4 16: 29: 56 6 9.25 8.02 17.6 110 K4
2347 LT 14398B 14: 51: 2.4 9: 43: 24 6 8.90 6.73 27.2 110 K4 C
2609 Gl 629.2A 16: 34: 42.4 -4: 13: 38 6 9.62 6.20 48.3 110 F8
2656 AG38:152 16: 50: 54.3 38: 9: 0 6 10.55 8.13 30.5 110 K3 B
2759 VV 251 A 17: 26: 10.6 1: 48: 20 3 10.90 5.09 145.0 0 G0
2768 Gl 677 A 17: 29: 20.2 29: 23: 33 6 9.55 7.69 23.6 110 K3
2807 Gl 690 A 17: 38: 34.3 71: 19: 53 6 9.20 7.31 23.9 110 K4
2856 Gl 700.1C 18: 3: 13.9 -8: 11: 25 1 9.40 5.91 50.0 0 G1 B
3022 LP336-6 19: 11: 5.9 32: 39: 59 3 10.48 0.48 1000.0 0 M0 III B
3030 Gl 748.2A 19: 14: 58.8 2: 9: 51 6 10.20 7.42 36.0 110 K2
3309 Wo 9723 21: 8: 46.4 47: 9: 25 6 10.78 6.64 67.4 110 K2
3315 GJ 2152 21: 13: 29.1 7: 26: 13 4 16.17 15.96 11.0 0 DA F
3438 +32 4292A 21: 55: 38.6 33: 2: 11 3 10.00 5.00 100.0 0 G0 B
3462 AC+01:2189 22: 3: 28.6 1: 35: 48 3 10.34 5.45 95.0 0 K1
3493 Wo 9775 22: 14: 24.1 -8: 44: 37 6 11.85 6.84 100.4 110 K1 B
3495 Gl 851.4 22: 14: 1.0 57: 7: 11 6 9.83 5.07 89.4 110 K0
3555 VV 271 22: 37: 11.9 0:-39: 1 3 10.50 5.98 80.0 0 G8 B
3585 +43 4306 22: 47: 31.6 44: 33: 11 3 9.60 3.72 150.0 0 G0 B
3692 Wo 9826 23: 25: 55.3 29: 11: 44 6 11.05 6.71 73.8 110 K1
3734 LP463-28B 23: 38: 58.6 21: 1: 23 2 16.40 14.33 26.0 0 DC C
3798 Wo 9848 0: 1: 54.9 26: 0: 20 6 11.30 8.10 43.6 110 K0

Names

Gl - Gliese (1969); GJ - Gliese & Jahreiss (1979); Wo - Woolley et al, (1970); LHS - Luyten Half-Second Catalogue; LTT - Luyten Two-Tenths Catalogue; PS - Pesch & Sanduleak (1978); Wo - Woolley et al (1970)


Notes

A: distance estimate taken from the pCNS3.
B: distance estimated from the spectral types.
C: distance estimated from the characteristics of the companion star.
D: NN 757 - foreground reddening is probably present.
E: NN 2053 - FS Comae - distance from Jura & Kleinmann's estimate of MK
F: white dwarf - distance from McCook & Sion's (MV, (B-V)) relations

Table 1D

NN Name RA (2000) Dec Ref MV Dist (pc) % D Spectral type
3804 RE0618+75 6: 18: 10.2 75: 6: 49 3 9.99 21.00 30 M 1.5
3805 Bonds star 23: 31: 7.5 -2: 45: 0 3 13.66 18.50 29 M 4.5
3806 Gl 129 3: 13: 44.7 18: 50: 37 2 11.70 32.40 8 sd K5
3809 LP355-60 13: 44: 0.0 -26: 18: 0 3 12.10 19.10 29 M 3.5
3810 BRI0021+02 0: 24: 21.4 2: 31: 29 2 18.31 13.80 3 M 9.5
3811 RE1816+54 18: 16: 25.9 54: 10: 34 4 12.02 39.40 30 M
3812 LHS 2090 9: 0: 23.5 21: 50: 5 5 17.10 6.00 18 M 6.5

References

Gliese, W. 1969, Veroff. Astr. Rechen-Instituts, Heidelberg, Nr. 22
Gliese, W. & Jahreiss, H. 1979, AAS, 38, 423
Luyten, W.J. 1979a, Catalogue of stars with proper motions exceeding 0"5 annually (LHS), Univ. of Minnesota Publ., Minneapolis, Minnesota
Luyten, W.J., Albers, H. 1979b, The LHS Atlas, Univ. of Minnesota Publ., Minneapolis, Minnesota
Reid, I.N. & Murray, C.A. 1991, AJ
Woolley, R. v.d.r., Epps, E.A., Penston, M.J., Pocock, S.B. 1970, Royal Obs. Ann., No. 5

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Neill Reid - last revised 23 June, 2001