All Tables

Table 1: Observational parameters of the data sets obtained with KOSMA. Columns one and two indicate the line and transition frequency, followed by the number of points, the spacing (the data on a sampling raster of 30'' were regridded on a 60'' raster), and half power beam width (HPBW) in arcsec; $\eta _{\rm mb}$ is the main-beam efficiency, $T_{\rm sys}$ the average system temperature, $\Delta v_{\rm res}$ denotes the channel spacing, and $\Delta T_{\rm rms}$ the average rms noise temperature (of the data on a 60'' grid) per channel on a $T_{\rm mb}$ scale.
Table C.1: Physical parameters of the clumps found in the ¹³CO 2 $\;\to\;$ 1 map of the CygX-North region. The columns indicate: (1) the running number of the clump shown in Figs. B.1-B.6; (2) the center velocity of the clump emission derived from the clump averaged ¹³CO 2 $\;\to\;$ 1 spectrum; (3) the line width of the ¹³CO spectrum averaged across the clump; (4) and (5) ¹²CO and ¹³CO 2 $\;\to\;$ 1 main beam brightness temperature determined at the position of peak emission; (6) excitation temperature derived from $T_{\rm mb}$ (¹²CO); (7) excitation temperature derived from the ¹³CO 3 $\;\to\;$ 2/2 $\;\to\;$ 1 line ratio; (8) opacity calculated from $T_{\rm mb}$ (¹³CO) and $T_{\rm ex12}$ ; (9) total ¹³CO column density; (10) H₂ column density; (11) mass of the clump; (12) Equivalent Radius (r = (area/ $\pi$ )^0.5 with the area determined by the polygon), deconvolved with the beamsize; and (13) average n(H₂) density, assuming a spherical cloud.
Table C.2: Physical parameters of the clumps found in the ¹³CO 2 $\;\to\;$ 1 map of the CygX-South region. The columns indicate: (1) the running number of the clump shown in Figs. B.1-B.6; (2) the center velocity of the clump emission derived from the clump averaged ¹³CO 2 $\;\to\;$ 1 spectrum; (3) the line width of the ¹³CO spectrum averaged across the clump; (4) and (5) ¹²CO and ¹³CO 2 $\;\to\;$ 1 main beam brightness temperature determined at the position of peak emission, crosses indicate positions where the ¹²CO 3 $\;\to\;$ 2 intensity is shown; (6) excitation temperature derived from $T_{\rm mb}$ (¹²CO); (7) excitation temperature derived from the ¹³CO 3 $\;\to\;$ 2/2 $\;\to\;$ 1 line ratio; (8) opacity calculated from $T_{\rm mb}$ (¹³CO) and $T_{\rm ex12}$ ; (9) total ¹³CO column density; (10) H₂ column density; (11) mass of the clump; (12) Equivalent Radius (r = (area/ $\pi$ )^0.5 with the area determined by the polygon), deconvolved with the beamsize; and (13) average n(H₂) density, assuming a spherical cloud.