Table 5.
Stellar and gas kinematics results, extracted within 1Rr.
| Name | V* | σ* | (V/σ)* | Vion | σion | (V/σ)ion | Vmol | σmol | (V/σ)mol |
|---|---|---|---|---|---|---|---|---|---|
| (km s−1) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| NGC 2369 (†) | 190 ± 16 | 118 ± 18 | 1.61 ± 0.30 | 164 ± 48 | 56 ± 2 | 2.91 ± 0.63 | 154 ± 10 | 53 ± 3 | 2.93 ± 0.24 |
| NGC 3110 | 143 ± 18 | 108 ± 18 | 1.32 ± 0.27 | 211 ± 44 | 40 ± 2 | 5.30 ± 0.87 | 216 ± 28 | 41 ± 2 | 5.20 ± 0.70 |
| ESO 320-G030 | 207 ± 13 | 86 ± 14 | 2.40 ± 0.41 | 244 ± 13 | 27 ± 4 | 9.16 ± 1.47 | 263 ± 40 | 47 ± 3 | 5.57 ± 0.92 |
| IRAS F12115-4656 | 163 ± 17 | 89 ± 13 | 1.83 ± 0.33 | 213 ± 12 | 34 ± 2 | 6.22 ± 0.51 | 217 ± 11 | 35 ± 11 | 6.14 ± 1.88 |
| IRAS F17138-1017 | 165 ± 10 | 87 ± 16 | 1.89 ± 0.35 | 172 ± 18 | 53 ± 3 | 3.23 ± 0.39 | 148 ± 12 | 46 ± 2 | 3.21 ± 0.28 |
| IC 4687 | 279 ± 40 | 79 ± 15 | 3.51 ± 0.96 | 328 ± 53 | 39 ± 3 | 8.34 ± 1.37 | 325 ± 62 | 36 ± 4 | 8.96 ± 1.84 |
| IC 5179 | 151 ± 33 | 92 ± 14 | 1.64 ± 0.41 | 161 ± 11 | 34 ± 4 | 4.68 ± 0.55 | 175 ± 16 | 32 ± 4 | 5.43 ± 0.79 |
Notes. Columns (2), (5), and (8): inclination-corrected velocity amplitude, defined as the value of the rotation curve at Rr. Columns (3), (6), and (9): aperture-smearing corrected velocity dispersion. Columns (4), (7), and (10): V/σ for the stellar, ionised, and molecular gas phases, respectively. Uncertainties were computed with Monte Carlo simulations. The ongoing merger (i.e. NGC 3256) was discarded from this analysis due to its limited FoV and peculiar kinematics. We also dismissed NGC 5135 and NGC 7130 due to their irregular velocity profiles, produced by their face-on orientations. (†)The emission lines of NGC 2369 were fitted using double-Gaussian profiles (see Sect. 4.3 and Appendix D) and its σ values were assumed to be the average of both components across the FoV. However, its complex kinematics does not allow us to extract a velocity amplitude and therefore we assume its value from the single-Gaussian map.
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