APEX and NOEMA observations of H2S in nearby luminous galaxies and the ULIRG Mrk 231 - A possible relation between dense gas properties and molecular outflows

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Table 4.

NOEMA observation results for Mrk 231.

		Core			Wings
Species	Transition	Line peak	I ^(a)	Δv	I_redwing ^(b)	I_bluewing ^(c)
		(mJy beam⁻¹)	(Jy kms⁻¹)	(kms⁻¹)	(Jy kms⁻¹)	(Jy kms⁻¹)
H₂S	1_1, 0–1_0, 1	7.08	1.69 ± 0.11	224.68 ± 29.48	0.07 ± 0.07	0.02 ± 0.07
HCN	J = 2–1	90.6	24.09 ± 0.14	255	1.74 ± 0.14	1.18 ± 0.14
HCO⁺	J = 2–1	68.0	15.58 ± 0.14	215	0.78 ± 0.14	1.09 ± 0.14

Notes. The values for HCN and HCO⁺ are taken from Lindberg et al. (2016).

^(a)

Integrated intensity between −250 and 250 km s⁻¹.

^(b)

Integrated intensity between 350 and 515 km s⁻¹ for H₂S, and between 350 and 990 km s⁻¹ for HCN and HCO⁺.

^(c)

Integrated intensity between −538 and −350 km s⁻¹ for H₂S, and between −990 and −350 km s⁻¹ for HCN and HCO⁺.

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