Table 1.
Sample of prolate rotators.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
|---|---|---|---|---|---|---|
| Name | Other names | Survey | Ψ | D | MK | log(MJAM) |
| (deg) | (Mpc) | (mag) | ||||
| NGC 1222 | A3D | 73 ± 15 (a) | 33.3 (f) | −22.71 | 10.50 (k) | |
| NGC 4261 | A3D | 74 ± 3 (a) | 30.8 (f) | −25.19 | 11.72 (k) | |
| NGC 4365 | VCC 731 | A3D | 76 ± 7 (a) | 23.3 (f) | −25.20 | 11.53 (k) |
| NGC 4406 | M 86 | A3D | 81 ± 13 (a) | 16.8 (f) | −25.03 | 11.60 (k) |
| NGC 4486 | M 87 | A3D | 46 ± 58 (a) | 17.2 (f) | −25.37 | 11.73 (k) |
| NGC 5557 | A3D, MAS | 73 ± 6 (a) | 38.8 (f) | −24.87 | 11.33 (k) | |
| NGC 5485 | A3D, CAL | 80 ± 3 (b) | 25.2 (f) | −23.61 | 11.06 (k) | |
| NGC 0647 | CAL | 72 ± 3 (b) | 184 (b) | – | (∼11.57) (b) | |
| NGC 0810 | CAL | 87 ± 2 (b) | 110 (b) | −25.67 | ∼11.7 | |
| NGC 2484 | CAL | 52 ± 4 (b) | 192 (b) | −26.56 | ∼12.1 | |
| NGC 4874 | CAL, MAS | 86 ± 5 (b) | 102 (b) | −26.19 | ∼12.0 | |
| NGC 5216 | Arp 104 | CAL | 66 ± 5 (b) | 42 (b) | −23.25 | ∼10.7 |
| NGC 6173 | CAL | 80 ± 2 (b) | 126 (b) | −26.14 | ∼11.9 | |
| PGC 021757 | LSBC F560–04 | CAL | 57 ± 5 (b) | 238 (b) | −26.79 | ∼12.2 |
| NGC 1052 | – | ∼90 (c) | 19.4 (g) | −24.00 | ∼11.0 | |
| NGC 2783 | UGC 04859 | MAS | 76 ± 11 (d) | 85.8 (h) | −25.35 | ∼11.6 |
| NGC 4589 | – | ∼45 (e) | 22.0 (g) | −23.96 | ∼11.0 | |
| NGC 7252 | Arp 226 | – | – | 60.1 (i) | −24.59 | ∼11.3 |
| PGC 018579 | AM 0609–331 | – | – | 129 (j) | −24.48 | ∼11.2 |
Notes. (1) The galaxy name in the NGC or PGC catalog; (2) An alternative galaxy name; (3) A3D, CAL, MAS – the galaxy is included in the ATLAS3D, CALIFA, or MASSIVE survey, respectively; (4) Ψ, the misalignment angle between the kinematic and photometric axis, where available; (5) D, the distance of the galaxy; (6) MK, total galaxy absolute magnitude (see Sect. 2.2); (7) log(MJAM), the dynamical mass of the galaxy – the ATLAS3D value is adopted where possible, the rest are approximate estimates calculated from a MK–log(MJAM) relation, except for NGC 0647, where the stellar mass estimate from Tsatsi et al. (2017) is listed instead (see Sect. 2.2).
ATLAS3D (Krajnović et al. 2011),
CALIFA (Tsatsi et al. 2017),
MASSIVE (Ene et al. 2018),
ATLAS3D (Cappellari et al. 2011),
MASSIVE (Ma et al. 2014),
ATLAS3D (Cappellari et al. 2013).
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