Table A.1
OH, HI, and H2 column densities
| OH 1667 MHz | OH 1665 MHz | OH 1612 MHz | OH 1720 MHz | HI | 12CO | 13CO | C18O | 13CO | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| J=1-0 | J=1-0 | J=1-0 | J=1-0 | ||||||||||||||||
| Source | vmid | RGC | ∫τdv | τmax | ∫τdv | τmax | ∫τdv | τmax | ∫τdv | τmax | ∫τdv | τmax | ![]() |
![]() |
∫ Tmb dv | ∫ Tmb dv | ∫ Tmb dv | ∫ Tmb dv | NH2 |
| [km s-1] | [kpc] | [km s-1] | [km s-1] | [km s-1] | [km s-1] | [km s-1] | ![]() |
![]() |
[K km s-1] | [K km s-1] | [K km s-1] | [K km s-1] | x1020cm-2 | ||||||
| G21.347-0.629 | +7.4 | 7.64 | +0.25 | +0.14 | +0.14 | +0.07 | <0.07 | <0.01 | +0.03 | +0.02 | >18.95 | >3.66 | 24.5 | 1.5 | <1.3 | 1.5 | 49.0 | ||
| +51.6 | 5.07 | +0.36 | +0.14 | +0.17 | +0.07 | +0.00 | +0.01 | +0.06 | +0.04 | >10.82 | >3.64 | 8.09 | >1.97 | 51.9 | 11.5 | <1.3 | 11.5 | 103.7 | |
| +56.5 | 4.87 | +0.50 | +0.37 | +0.32 | +0.28 | -0.04 | +0.00 | +0.15 | +0.13 | >9.04 | >3.70 | 11.17 | >1.65 | 22.2 | 9.7 | 2.9 | 9.7 | 44.5 | |
| +73.5 | 4.24 | +0.13 | +0.04 | +0.06 | +0.03 | +0.04 | +0.02 | <0.06 | <0.01 | +7.31 | +1.38 | 2.86 | 1.33 | 16.1 | <1.3 | <1.3 | <1.3 | 32.1 | |
| +68.8 | 4.41 | +0.05 | +0.06 | +0.02 | +0.03 | <0.02 | <0.01 | <0.02 | <0.01 | +0.58 | +0.36 | 1.13 | 0.11 | <2.4 | <1.3 | <1.3 | <1.3 | <4.9 | |
| +66.6 | 4.48 | +0.05 | +0.05 | +0.03 | +0.03 | <0.02 | <0.01 | <0.02 | <0.01 | +0.50 | +0.27 | 1.07 | 0.09 | 2.2 | <1.3 | <1.3 | <1.3 | 4.4 | |
| G29.957-0.018 | +6.5 | 7.87 | +0.19 | +0.12 | +0.11 | +0.07 | +0.08 | +0.06 | -0.03 | +0.01 | +4.19 | +1.56 | 4.27 | 0.76 | 12.9 | 2.2 | <1.3 | 2.2 | 25.8 |
| +9.7 | 7.68 | +0.08 | +0.07 | +0.05 | +0.04 | +0.04 | +0.03 | <0.02 | <0.01 | +2.67 | +1.14 | 1.84 | 0.49 | 2.6 | <1.3 | <1.3 | <1.3 | 5.1 | |
| +67.5 | 5.18 | +0.10 | +0.03 | +0.05 | +0.02 | +0.04 | +0.02 | <0.06 | <0.01 | +7.55 | +1.26 | 2.15 | 1.38 | 21.9 | 4.3 | <1.3 | 4.3 | 43.8 | |
| +97.8 | 4.32 | +0.14 | +0.06 | +0.09 | +0.04 | -0.03 | +0.02 | +0.08 | +0.06 | >13.24 | >3.59 | 3.18 | >2.41 | 160.6 | 63.9 | 13.9 | 63.9 | 321.1∗ | |
| +102.8 | 4.19 | +0.14 | +0.06 | -0.25 | +0.01 | -0.19 | +0.00 | +0.16 | +0.07 | >12.18 | >3.59 | 3.21 | >2.22 | 87.1 | 24.6 | 4.4 | 24.6 | 174.1∗ | |
| 12CO | 13CO | C18O | |||||||||||||||||
| J=2–1 | J=2–1 | J=2–1 | |||||||||||||||||
| G29.935-0.053 | +7.5 | 7.81 | +0.15 | +0.07 | +0.09 | +0.05 | +0.08 | +0.05 | <0.12 | <0.04 | +5.53 | +1.29 | 3.47 | 1.01 | 3.4 | 0.4 | <0.2 | <1.3 | 9.8 |
| +50.8 | 5.77 | +0.29 | +0.14 | +0.13 | +0.06 | <0.12 | <0.04 | <0.11 | <0.04 | >11.84 | >2.64 | 6.39 | >2.16 | 22.5 | 5.6 | 0.8 | 7.8 | 64.3 | |
| +68.0 | 5.17 | +0.20 | +0.14 | +0.13 | +0.09 | +0.09 | +0.05 | <0.08 | <0.04 | >8.30 | >2.62 | 4.56 | >1.51 | 9.9 | 1.1 | <0.2 | 3.2 | 28.4 | |
| +99.0 | 4.29 | +0.76 | +0.26 | +0.64 | +0.18 | -0.07 | +0.03 | +0.27 | +0.08 | >18.10 | >2.64 | 17.07 | >3.30 | 113.7 | 58.1 | 18.2 | 72.3 | 377.5a,* | |
| G31.388-0.383 | -3.8 | 8.54 | +0.10 | +0.07 | +0.04 | +0.03 | +0.03 | +0.02 | <0.03 | <0.02 | +1.16 | +0.57 | 2.27 | 0.21 | 1.5 | 0.2 | <0.2 | <0.9 | 4.3 |
| +18.0 | 7.25 | +0.22 | +0.14 | +0.11 | +0.08 | +0.04 | +0.03 | +0.02 | +0.02 | >22.74 | >3.89 | 4.98 | >4.14 | 7.6 | 0.6 | <0.2 | <0.9 | 21.8 | |
| +37.0 | 6.38 | +0.03 | +0.04 | <0.03 | <0.02 | <0.03 | <0.02 | <0.03 | <0.02 | +2.15 | +0.88 | 0.74 | 0.39 | 0.3 | <0.2 | <0.2 | <0.9 | 0.8 | |
| +73.1 | 5.11 | +0.12 | +0.04 | +0.06 | +0.03 | +0.07 | +0.02 | -0.06 | +0.00 | +17.18 | +3.59 | 2.58 | 3.13 | 7.3 | 0.5 | <0.2 | 2.5 | 20.9 | |
| +78.1 | 4.96 | +0.12 | +0.12 | +0.07 | +0.07 | +0.03 | +0.02 | +0.01 | +0.02 | +5.67 | +2.39 | 2.64 | 1.03 | 2.0 | 0.2 | <0.2 | 0.7 | 5.8 | |
| +81.8 | 4.85 | +0.06 | +0.04 | <0.03 | <0.02 | <0.03 | <0.02 | <0.03 | <0.02 | >11.84 | >3.85 | 1.37 | >2.16 | 3.6 | 0.4 | <0.2 | 1.0 | 10.4 | |
| +85.3 | 4.75 | +0.11 | +0.07 | +0.03 | +0.03 | <0.03 | <0.02 | +0.03 | +0.02 | >13.04 | >3.87 | 2.53 | >2.38 | 2.8 | 0.2 | <0.2 | 0.4 | 7.9 | |
| +92.0 | 4.57 | +0.05 | +0.04 | +0.04 | +0.02 | <0.03 | <0.01 | <0.03 | <0.02 | +6.65 | +2.47 | 1.19 | 1.21 | 4.7 | 0.5 | <0.2 | 1.5 | 13.4 | |
Notes. Integral and peak of the optical depth of the OH and H I lines, as well as of integrated CO emission. As we do not derive the excitation temperatures of the OH and H I lines in this work, we report NOH/Tex and NHI/TS. (*) Features associated with HII regions. All other features are line-of-sight absorption features. (a) Using 13CO J = 1 - 0 and correcting for isotope ratio variations over Galactocentric distance (Sect. 3.2).
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