ATLASGAL-selected massive clumps in the inner Galaxy - VIII. Chemistry of photodissociation regions

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Volume 644 (December 2020)

A&A, 644 (2020) A160

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Table 4

Gaussian line parameters of C¹⁸O, HCO, H¹³CO⁺, c-C₃ H₂, CN, HC¹⁵N, and HN¹³C.

ATLASGAL	Line	Area	v_LSR	Δv	T_MB	rms
name		(K km s⁻¹)	(km s⁻¹)	(km s⁻¹)	(K)	(K)
AGAL008.671−00.356	HCO	0.83 ± 0.10	36.43 ± 0.48	6.57 ± 0.78	0.12	0.03
	H¹³CO⁺	11.93 ± 0.91	34.20 ± 0.06	3.07 ± 0.10	3.65	0.05
	c-C₃H₂	5.40 ± 0.33	36.29 ± 0.18	5.73 ± 0.26	0.88	0.05
	HN¹³C	10.12 ± 0.14	35.25 ± 0.03	4.47 ± 0.07	2.13	0.05

AGAL010.151−00.344	C¹⁸O	17.65 ± 0.09	9.19 ± 0.01	5.48 ± 0.03	3.03	0.03
	HCO	0.86 ± 0.08	8.70 ± 0.36	7.42 ± 0.75	0.10	0.02
	H¹³CO⁺	7.98 ± 0.11	9.50 ± 0.04	5.26 ± 0.09	1.43	0.04
	c-C₃H₂	8.24 ± 0.10	9.48 ± 0.03	4.99 ± 0.07	1.55	0.03
	CN	5.06 ± 0.16	9.34 ± 0.08	5.18 ± 0.19	0.92	0.06
	HC¹⁵N	0.35 ± 0.09	10.65 ± 0.33	2.99 ± 1.07	0.11	0.04
	HN¹³C	3.13 ± 0.10	9.49 ± 0.07	4.43 ± 0.16	0.66	0.04

Notes. For multiplevelocity components, we only tabulate line parameters of the component detected in all molecular species. The full table is available at the CDS.

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