Table B.1
SpDust input parameters for the spectra in Fig. B.1 and best-fit parameters for the CCA spectral model.
| SpDust | CCA | |||||||
| Model name | nH [cm-3] | T[K] | χ | x H | x C | ν p | m 60 | |
|
|
||||||||
| WNM | 0.4 | 6000 | 1.00 | 0.10 | 0.0003 | 24.22 | 7.53 | |
| CNM | 30.0 | 100 | 1.00 | 0.0012 | 0.0003 | 29.00 | 4.93 | |
| WIM | 0.1 | 8000 | 1.00 | 0.99 | 0.001 | 27.30 | 5.66 | |
| MC | 300 | 20 | 0.01 | 0.0 | 0.0001 | 38.77 | 2.00 | |
Notes. The SpDust input parameters are the total hydrogen number density nH, the gas temperature T, the intensity of the radiation field relative to the average interstellar radiation field χ, the hydrogen ionization fraction xH = nH + /nH, and the ionized carbon fractional abundance xC = nC + /nH.
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