Table 1.
Targets’ physical parameters.
| Name | Type | D | SFR | log(LX) | log(L1.4 GHz) | S(CO)32 | Bar | z | RA | Dec |
|---|---|---|---|---|---|---|---|---|---|---|
| Mpc | M⊙/yr | erg/s | W/Hz | Jy km s−1 | PA(°) | ICRS | ICRS | |||
| N613 | Sy- SB(rs)bc | 17.2 | 5.3 | 41.2 | 21.8 | 56. | 127 | 0.00494 | 01:34:18.189 | −29:25:06.59 |
| N1672 | Sy 2- SB(s)b | 11.4 | 3.1 | 38.4 | 19.9 | 80. | 97 | 0.00444 | 04:45:42.496 | −59:14:49.91 |
Notes. D are the median values of z-independent distances from NED (Steer et al. 2017). SFRs are derived from infrared luminosities (NED). LX is from 2 to 10 keV INTEGRAL, Rosat, and/or Chandra archives. The CO(3–2) integrated fluxes are from the molecular torus only (Combes et al. 2019). PA of bars are from Jungwiert et al. (1997) for NGC 613, and from Jenkins et al. (2011) for NGC 1672. The RA-Dec positions are the adopted centers for each galaxy, derived from the continuum point sources detected with ALMA, with an error bar of ∼0.1″ (Combes et al. 2019).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.