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 1.

Basic information of sources.

Galaxy	α (J 2000)	δ (J 2000)	D ^(a)	L_IR ^(b)	Type	Outflow ^(c)	Water vapour ^(d)	t_int ^(e)	rms[LSB/USB] ^(f)
	(h:m:s)	(° : ′: ″)	(Mpc)	(L_⊙)				(hours)	(mK)
NGC 253	00:47:33.1	−25:17:18	03.1	3.0 × 10¹⁰	SB	00Yes⁽¹⁾	No	1.5	0.48/0.87
NGC 1068	02:42:40.7	−00:00:48	13.7	2.0 × 10¹¹	AGN+SB	00Yes⁽²⁾	No	3.5	0.35/0.60
NGC 1097	02:46:19.0	−30:16:30	16.8	5.0 × 10¹⁰	LLAGN	No	No	1.2	0.30/0.51
NGC 1377	03:36:39.1	−20:54:08	23.66	1.3 × 10¹⁰	AGN?	00Yes⁽³⁾	No	7.7	0.24/0.60
NGC 3256	10:27:51.3	−43:54:13	35.35	3.6 × 10¹¹	SB	00Yes⁽⁴⁾	0Yes⁽¹⁾	6.9	0.20/0.38
NGC 4418	12:26:54.6	−00:52:39	31.9	1.0 × 10¹¹	AGN	00Yes⁽⁵⁾	0Yes⁽²⁾	1.1	0.41/0.67
Mrk 231	12:56:14.2	+56:52:25	171.8	3.2 × 10¹²	AGN+SB	00Yes⁽⁶⁾	0Yes⁽³⁾		0.6(mJy beam⁻¹)/ –
NGC 4826	12:56:43.6	+21:40:59	03.1	4.0 × 10⁹	AGN	No	No	2.8	0.27/0.66
NGC 4945	13:05:27.5	−49:28:06	03.9	3.0 × 10¹⁰	AGN/SB	00Yes⁽⁷⁾	No	4.9	0.46/1.0
IC 860	13:15:03.5	+24:37:08	59.1	1.5 × 10¹¹	LIRG	00Yes⁽⁸⁾	0Yes⁽⁴⁾	2.6	0.52/0.80
NGC 5128	13:25:27.6	−43:01:09	04.0	2.0 × 10¹¹	AGN	00Yes⁽⁹⁾	No	1.4	–/–
M 83	13:37:00.9	−29:51:56	03.6	1.0 × 10¹⁰	SB	No	No	1.4	0.51/0.96
Circinus	14:13:09.9	−65:20:21	04.2	6.9 × 10¹⁰	AGN/SB	00Yes⁽¹⁰⁾	No	3.5	0.37/0.81

Notes.

^(a)

Distances are taken from Sanders et al. (2003) except for Circinus, whose value was taken from the NASA/IPAC Extragalactic Database.

^(b)

Infrared luminosities taken from Sanders et al. (2003) except for that of Circinus, which was calculated from the flux densities of 12 μm, 25 μm, 60 μm, and 100 μm taken from Brauher et al. (2008, Table 1).

^(c)

Presence of molecular outflow report. (1) e.g. Bolatto et al. (2013a), Walter et al. (2017), (2) e.g. Emsellem et al. (2006), Barbosa et al. (2014), García-Burillo et al. (2015), (3) e.g. Aalto et al. (2012, 2016),(4) e.g. Sakamoto et al. (2014), Michiyama et al. (2018), (5) e.g. Ohyama et al. (2019), (6) e.g. Spoon et al. (2013), (7) Henkel et al. (2018), (8) e.g. Aalto et al. (2019) (9) e.g. Israel et al. (2017), (10) Curran et al. (1999), Zschaechner et al. (2016).

^(d)

Presence of water detection. (1) Herschel SPIRE data, (2) González-Alfonso et al. (2012), and Herschel SPIRE data, (3) González-Alfonso et al. (2010), (4) Herschel PACS data.

^(e)

On-source observation time.

^(f)

Noise level obtained from the CLASS (http://www.iram.fr/IRAMFR/GILDAS).

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