Exploring the interplay between molecular and ionized gas in H II regions

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Table C.3

Derived physical properties of molecular clouds.

GLOSTAR	ATLASGAL	Comp¹	T_kin [K]	log10(n_H₂) [cm⁻³]	log10(N_{para–H₂CO}) [cm⁻²]	log10(X_{para–H₂CO)}	log10(N_H₂) [cm⁻²]
G3.350–0.077	AGAL003.351–00.077	a	${111.25}_{- 0.49}^{+ 1.89}$ $\[111.25_{-0.49}^{+1.89}\]$	${4.97}_{- 0.73}^{+ 0.51}$ $\[4.97_{-0.73}^{+0.51}\]$	${13.43}_{- 0.36}^{+ 0.6}$ $\[13.43_{-0.36}^{+0.6}\]$	−8.59	22.02
G3.350–0.077	AGAL003.351–00.077		${47.2}_{- 0.92}^{+ 1.1}$ $\[47.2_{-0.92}^{+1.1}\]$	${5.44}_{- 0.13}^{+ 0.12}$ $\[5.44_{-0.13}^{+0.12}\]$	${13.69}_{- 0.08}^{+ 0.09}$ $\[13.69_{-0.08}^{+0.09}\]$	−8.32	22.02
G6.552–0.095	AGAL006.551–00.097		${40.24}_{- 0.86}^{+ 1.15}$ $\[40.24_{-0.86}^{+1.15}\]$	${5.71}_{- 0.18}^{+ 0.18}$ $\[5.71_{-0.18}^{+0.18}\]$	${13.05}_{- 0.08}^{+ 0.09}$ $\[13.05_{-0.08}^{+0.09}\]$	−9.12	22.17
G6.552–0.095	AGAL006.551–00.097	a	${59.25}_{- 0.87}^{+ 1.21}$ $\[59.25_{-0.87}^{+1.21}\]$	${5.14}_{- 0.43}^{+ 0.19}$ $\[5.14_{-0.43}^{+0.19}\]$	${13.57}_{- 0.14}^{+ 0.35}$ $\[13.57_{-0.14}^{+0.35}\]$	−8.61	22.17
G7.472+0.058	AGAL007.471+00.059		${52.11}_{- 0.88}^{+ 1.23}$ $\[52.11_{-0.88}^{+1.23}\]$	${5.17}_{- 0.72}^{+ 0.2}$ $\[5.17_{-0.72}^{+0.2}\]$	${13.74}_{- 0.15}^{+ 0.61}$ $\[13.74_{-0.15}^{+0.61}\]$	−8.55	22.29
G7.177+0.088	AGAL007.178+00.086		${54.77}_{- 0.88}^{+ 1.15}$ $\[54.77_{-0.88}^{+1.15}\]$	${5.49}_{- 0.16}^{+ 0.14}$ $\[5.49_{-0.16}^{+0.14}\]$	${13.52}_{- 0.08}^{+ 0.1}$ $\[13.52_{-0.08}^{+0.1}\]$	−7.25	20.77
G8.669–0.355	AGAL008.671–00.356		${145.45}_{- 0.72}^{+ 1.42}$ $\[145.45_{-0.72}^{+1.42}\]$	${5.33}_{- 0.43}^{+ 0.27}$ $\[5.33_{-0.43}^{+0.27}\]$	${14.53}_{- 0.14}^{+ 0.28}$ $\[14.53_{-0.14}^{+0.28}\]$	−7.68	22.21
G8.669–0.355	AGAL008.671–00.356	a	${121.81}_{- 0.67}^{+ 1.42}$ $\[121.81_{-0.67}^{+1.42}\]$	${5.94}_{- 0.24}^{+ 0.8}$ $\[5.94_{-0.24}^{+0.8}\]$	${14.09}_{- 0.03}^{+ 0.07}$ $\[14.09_{-0.03}^{+0.07}\]$	−8.13	22.21
G8.669–0.355	AGAL008.671–00.356	b					22.21
G9.875–0.749	AGAL009.879–00.751	a					21.63

Notes. ¹a, b, c: indicates the secondary velocity components.

The table presents the first ten sources from our sample. The entire table is accessible at the CDS.

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