|C I||C I||p|
|(Jy km s-1)||(Jy km s-1)||(1017 cm-2)|
|Tk||50 K||100 K||50 K||100 K|
Notes. Model A: , g/d = 100; B: , g/d = 10; C: Kurucz A3, g/d = 10; Thick: flux for optically thick lines. Predictions are for an assumed local line width of 0.2 km s-1. Model J is from Jonkheid et al. (2007), their model B4. All the line fluxes are scaled for a source distance of 140 pc. and p are the results of the power-law fitting of the modeled C I surface densities (Fig. 3).
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