Table 1
Different environments in the Galaxy: filling factors and CO clump properties.
| Env | q lbv | T HI | f CO | T COsig,HI | T COsig,CO | ε |
|
|
||||||
| 0:all | 1.000 | 22 | 1.13 | 68 | 1.30 | 0.68 |
| 1:inner bubble | 0.028 | 12 | 0.67 | 46 | 1.42 | 0.76 |
| 2:outer bubble | 0.026 | 22 | 1.99 | 40 | 1.45 | 0.79 |
| 3:inner wall | 0.209 | 30 | 2.34 | 60 | 1.26 | 0.70 |
| 4:outer wall | 0.204 | 32 | 1.49 | 72 | 1.30 | 0.66 |
| 5:outside | 0.200 | 25 | 1.06 | 86 | 1.38 | 0.63 |
| 6:outside | 0.182 | 13 | 0.28 | 85 | 1.29 | 0.63 |
| 7:outside | 0.150 | 4 | 0.02 | 38 | 0.77 | 0.79 |
Notes. The first part gives the type of the environment and its fraction in the whole datacube. The second part gives the average HI temperature in the environment and the CO filling factor (in %). The third part gives average HI and CO temperatures in pixels with the significant CO emission in the environment and their average molecularization.
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