All Tables

Table 1: List of observational parameters for KOSMA.
Table 2: Positions of ISO observations in absolute coordinates.
Table 3: Line-integrated intensities in [ ${\rm K}~{\rm km}~{\rm s}^{-1}$ ] (upper table) and in [10^-7 erg s^-1 cm^-2 sr^-1] (lower table) of the low- and mid-J CO isotopomeric lines and of the CS 7-6 line observed at KOSMA and FCRAO. In order to prevent the $+9~~{\rm km}~{\rm s}^{-1}$ velocity component from adding to the integrated intensity, the listed intensities were integrated only over the $-3~~{\rm km}~{\rm s}^{-1}$ component. As the ¹²CO lines merge with the second velocity component, these spectra were fitted using a 2-component Gaussian with the $+9~~{\rm km}~{\rm s}^{-1}$ velocity component masked out. All line intensities are reported for 80'' angular resolution (higher angular resolution data have been smoothed).
Table 4: The ISO/LWS high-J CO and atomic FIR lines at 80'' resolution. The transformation between flux densities and surface brightnesses was made using the beam sizes given in Table 5.10 of the ISO-LWS Handbook v. 2.1. The beam solid angle varies between $8\times 10^{-8}$ sr and $1.4\times 10^{-7}$ sr. Because the lines are unresolved, the line widths were held to the instrumental line width: 0.29 or 0.60 $\mu$ m for detectors 0-4 and 5-9, respectively. Correction factors between 0.37 to 0.85 for extended sources have been applied. We assume a 30% absolute photometry uncertainty for LWS.
Table 5: Results of dust continuum single-component fit, with $\beta$ fixed at 1.5, and $\Omega$ is $1.5\times 10^{-7}$ sr.
Table 6: C I and ¹³CO line ratio R (in ${\rm K}~{\rm km}~{\rm s}^{-1}$ ; values taken from Table 3), excitation temperature (with lower and upper $1\sigma$ limits), and C I, ¹³CO (with relative upper and lower errors), and C¹⁸O column densities (bracketed by $T_{\rm ex}$ of ¹³CO). All abundances X are relative to the H₂ column densities (first row; taken from Col. 4 of Table 5).
Table 7: The physical parameters for the observed ISO/LWS positions. The radii listed in Col. 2 give the inner and outer edge of each shell. Columns 3 to 7 lists the temperature, clump-averaged number density of H₂, volume filling, column density of H₂, and the gas mass. For these columns, the first entry is the mass-averaged value for the whole cloud, values in parentheses show averages within each shell. The last column lists the reduced $\chi ^2$ fit result for 11 lines (6 KOSMA, 2 FCRAO and 3 ISO).
Table 8: Total cooling intensities of CO, [C I], [C II], and [O I]. The values in parentheses show the relative contribution to the sum $I_{\rm tot}$ . The total cooling efficiency $\epsilon _{\rm tot}$ is defined by $I_{\rm tot}/I_{\rm IR}$ . For comparison, we also list the $\epsilon '$ defined by $(I_{\rm [C {\sc ii}]}+I_{\rm [O {\sc i}]})/I_{\rm IR}$ .