All Tables

Table 1: Parameters of the observed transitions used to study the PDRs in Cepheus B.
Table 2: Velocity components derived from Gaussian fitting of spectra at the position of the hotspot in Cepheus B.
Table 3: KOSMA- $\tau$ calculations of H₂, C and CO column densities of spherical clumps with n=10⁵ cm^-3 and $\chi = 10^2$ (Draine units). The column densities are for individual clumps, and not the column densities observed per beam.
Table 4: Results of PDR model calculations for ensembles of clumps having same mass and density. $\phi _{\rm A}$ is the area filling factor of the clumps.