All Tables

Table 1: Properties of the KOSMA- $\tau$ PDR-model clumps with given masses and densities at an incident FUV-flux of 10² $\ensuremath {\chi _{\rm D}}$ . Orders of magnitude are given in parentheses.
Table 2: The parameter values of the precomputed KOSMA- $\tau$ PDR-model clumps are equidistant on logarithmic scale in steps of half an order of magnitude.
Table 3: The fixed parameter values of the precomputed KOSMA- $\tau$ PDR-model clumps. Note that powers of ten are given in parentheses and the elemental abundances are given in units of the hydrogenabundance, i.e. X_i = n_i / n.
Table 4: Parameters of the Galaxy model (values at the solar circle).
Table 5: The parameter values used for the escape probability calculation of the [C II] ²[][3/2]P- ²[][1/2]P emissivity from the CNM and WNM. Powers of ten are given in parentheses.