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Table 1

Main properties of the galaxies.

Galaxy α (J 2000) δ (J 2000) Da VLSRb θsc SFRd Activity type
h:m:s °::′′ Mpc km s-1 ′′ /pc M yr-1 L

M 83 13:37:00.93 –29:51:56.40 4.5 513 15/327 2.5 1.2 × 1010 Starburst
NGC 253 00:47:33.12 –25:17:18.60 3.9 250 20/378 3.6 2.8 × 1010 Starburst
M 82-NE 09:55:51.90 69:40:47.00 3.5 300 12 /204 10 5.9 × 1010 Starburst
M 51 13:29:52.70 47:11:43.00 8.4 470 15/611 2.5 2.6 × 1010 AGN
NGC 1068 02:42:40.90 –00:00:46.00 14.4 1100 4/279 0.4 1.9 × 1011 AGN + Starburst
NGC 7469 23:03:15.60 08:52:26.00 29.5 4892 6/858 30 3.9 × 1011 AGN + Starburst
Arp 220 15:34:57.08 23:30:11.30 70.0 5350 2/679 240 1.6 × 1012 Starburst
Mrk 231 12:56:14.20 56:52:25.00 170.0 12 173 2/1640 220 3.2 × 1012 AGN

Notes. For M 82 we observed the north-eastern (NE) molecular lobe at an offset position (Δα,Δδ) = ( + 13.0′′, + 7.5′′) with respect to its dynamical centre.

(a)

Distances taken from the NASA/IPAC Extragalactic Database;

(b)

systemic local standard of rest (LSR) radial velocities following the optical convention, taken from SIMBAD;

(c)

source sizes and their corresponding spatial scales for the assumed distances;

(d)

star formation rate obtained from Walter et al. (2008) for M 83; Strickland et al. (2004) for NGC 253 and M 82; Schuster et al. (2007) for M 51; Esquej et al. (2014) for NGC 1068; Genzel et al. (1995) for NGC 7469; Anantharamaiah et al. (2000) for Arp 220; Taylor et al. (1999) for Mrk 231. We note that this parameter is only meant to give a rough idea of the activity, as it was calculated for different volumes in each galaxy. e Infrared luminosities taken from Sanders et al. (2003).

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