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Table D.1

Conditions in diffuse cloud models and coefficients for departure from LTE of the population in the CH N = 1, J = 1∕2 HFS.

Model 1 Model 2
diffuse molecular translucent
χ [Habing] 1.7 1.7
AV 0.2 1
nH [cm−3] 100 1000
0.1 0.5
Tgas [K] 100 15
Tdust[K] 16 12
ΔυFWHM [km s−1] 3.3 3.3
N(CH) [1013 cm−2] 1.75 1.58

LTE departure coefficients

F = 0+ 3.702 0.5480
F = 1+ 3.721 0.5492
F = 0− 6.875 2.178
F = 1− 6.948 2.199

Fractional population (per sub-level) in ground state

F = 0+ 0.0870 0.0504
F = 1+ 0.0875 0.0505
F = 0− 0.1613 0.1981
F = 1− 0.1630 0.2000

Fractional population in excited states [ppm]

100 200

Notes. Departure coefficients are defined as the fractional level population with respect to LTE. The FUV field is parametrized in units of the Habing field (Draine field = 1.7 Habing, Draine 1978).

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