Table 1.
Characteristics of the sample.
| Name | Type | D | SFR | log(LX) | log(L1.4 GHz) | S(CO)21 | Bar | Double | RA | Dec |
|---|---|---|---|---|---|---|---|---|---|---|
| Mpc | M⊙ yr−1 | erg s−1 | W Hz−1 | Jy km s−1 | PA(°) | bar? | ICRS | ICRS | ||
| N613 | Sy- SB(rs)bc | 17.2 | 5.3* | 41.2 | 21.8 | 1200a | 127 | 122 | 01:34:18.189 | −29:25:06.59 |
| N1326 | LINER- SB0(r) | 14.9 | 1.1 | 39.9 | 20.9 | 200b | 30 | 90 | 03:23:56.416 | −36:27:52.68 |
| N1365 | Sy 1.8- SB(s)b | 17.8 | 17. | 41.8 | 22.3 | 2300c | 92 | 46 | 03:33:36.368 | −36:08:25.51 |
| N1433 | Sy 2- SB(r)ab | 9.7 | 0.5 | 39.2 | 20.0 | 360a | 95 | 32 | 03:42:01.49 | −47:13:20.2 |
| N1566 | Sy 1.5- SAB(s)bc | 7.2 | 0.8 | 40.5 | 21.3 | 540a | 5 | No | 04:20:00.395 | −54:56:16.61 |
| N1672 | Sy 2- SB(s)b | 11.4 | 3.1 | 38.4 | 19.9 | 1140a | 97 | No | 04:45:42.496 | −59:14:49.91 |
| N1808 | Sy 2- SAB(s)a | 9.3 | 4.7 | 39.8 | 21.7 | 4500d | 139 | 158 | 05:07:42.329 | −37:30:45.85 |
Notes. D are the median values of z-independent distances from NED (Steer et al. 2017). SFR are derived from infrared luminosities (NED). ( * )NGC 613 has an H2O maser. LX is from 2–10 keV INTEGRAL, Rosat, and/or Chandra archives. The CO(2-1) integrated fluxes are from single-dish measurements (SEST, beam 22″) from (a)Bajaja et al. (1995), (b)Garcia-Barreto et al. (1991), (c)Sandqvist (1999), (d)Aalto et al. (1994). PA of bars are from Jungwiert et al. (1997) for NGC 613 and 1433, from Garcia-Barreto et al. (1991) for NGC 1326, Lindblad (1999) for NGC 1365, Agüero et al. (2004) for NGC 1566, Jenkins et al. (2011) for NGC 1672, and Dahlem et al. (1994) for NGC 1808. The RA-Dec positions are the new adopted centers for each galaxy, derived from the detected continuum point sources in the present work, with an error bar of ∼0.1″ (Sect. 4.1).
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