Table 1
Properties of the galaxy sample.
| Galaxy | αJ2000 | δJ2000 | RC3 type | Nuclear act. | D | i | PA | Gas morph.a | Gas mot. | Envir. | NUGA Ref. |
| [hms] | [°′′′] | [Mpc] | [deg] | [deg] | |||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
|
|
|||||||||||
| NGC 3627 | 11 20 15.02 | 12 59 29.5 | SAB(s)b | LINER/Seyfert 2 | 10.2 (1′′ = 49 pc) | 61 | 178 | Bar | Inflow | Interacting | (1) |
| NGC 4569 | 12 36 49.80 | 13 09 46.3 | SAB(rs)ab | Transition 2 | 16.8 (1′′ = 81 pc) | 62 | 15 | Bar | Inflow | Isolated | (2, 3) |
| NGC 4579 | 12 37 43.52 | 11 49 05.5 | SAB(rs)b | LINER/Sy1.9 | 19.8 (1′′ = 96 pc) | 36 | 95 | Spiral arms | Inflow | Isolated | (4, 5) |
| NGC 4826 | 12 56 43.64 | 21 40 59.3 | (R)SA(rs)ab | LINER | 5.4 (1′′ = 26 pc) | 54 | 112 | Disk | − | Isolated | (3, 4, 6) |
Notes.
Molecular gas morphology as revealed from NUGA IRAM 12CO(1−0) observations. For 12CO(2−1) and 12CO(3−2) morphologies we refer to NUGA papers.
Reference. (1) Casasola et al. (2011); (2) Boone et al. (2007); (3) Boone et al. (2011); (4) García-Burillo et al. (2005); (5) García-Burillo et al. (2009); (6) García-Burillo et al. (2003).
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