Table 6.
Dynamical and stellar mass estimations.
| Name |
 |
 |
 |
CAD |
 |
 |
|---|---|---|---|---|---|---|
| (1010 M⊙) | (1010 M⊙) | (1010 M⊙) | (1010 M⊙) | (1010 M⊙) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| NGC 2369 | 1.0 ± 0.3 | 0.6 ± 0.1 | 0.5 ± 0.1 | 1.6 ± 0.7 | 0.7 ± 0.2 | 1.7 ± 0.5 |
| NGC 3110 | 0.9 ± 0.3 | 1.2 ± 0.5 | 1.3 ± 0.3 | 1.0 ± 0.8 | 0.7 ± 0.2 | 2.1 ± 0.6 |
| ESO 320-G030 | 1.3 ± 0.2 | 1.4 ± 0.1 | 1.7 ± 0.5 | 1.9 ± 0.7 | 0.8 ± 0.2 | 2.7 ± 0.8 |
| IRAS F12115-4656 | 1.7 ± 0.5 | 2.1 ± 0.2 | 2.2 ± 0.2 | 1.6 ± 1.1 | ... | ... |
| IRAS F17138-1017 | 1.2 ± 0.3 | 1.0 ± 0.2 | 0.8 ± 0.2 | 2.1 ± 0.8 | 0.8 ± 0.2 | 3.2 ± 0.9 |
| IC 4687 | 2.6 ± 0.9 | 3.2 ± 1.0 | 3.2 ± 1.2 | 1.4 ± 0.8 | 0.8 ± 0.2 | 2.8 ± 0.9 |
| IC 5179 | 1.3 ± 0.6 | 1.1 ± 0.2 | 1.3 ± 0.2 | 1.1 ± 1.1 | 0.8 ± 0.2 | 3.9 ± 1.2 |
Notes. Columns (2)–(4): dynamical masses within 1Rr based on the stellar, ionised, and hot molecular gas kinematics. Column (5): values of the asymmetric-drift correction factor, as defined in Eq. (4). Columns (6) and (7): stellar masses estimated using a constant IRAC/3.6 μm M/L derived from the U et al. (2012) and Pereira-Santaella et al. (2015) results, respectively.
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