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We present here lists of some of the more important atomic and molecular lines in the infrared. It is by no means exhaustive.
(Nu - Nl)
Vacuum Wavelength
Vacuum Frequency
(cm -1)
Te=Ne=104

1

(Nu-Nl)
(cm -1)
Te=104
λ (μm)
(Nu-Nl)
12C16O
(cm -1)
13C16O
(cm -1)

1

Table B.13: Important H2 Lines
(μm)
(cm-1)
Eupper
(10e-7s)

1


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