Table 1.
Basic properties of the 6 galaxies studied in this paper.
| FCC ID | Name | Type | Distance | log(Mdyn) | Reff | σ | BT |
|---|---|---|---|---|---|---|---|
| Mpc | M⊙ | ″ | km s−1 | mag | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| FCC47 | NGC 1336 | E4 | 18.3 | 10.4 | 30.0 | 96.0 | 13.3 |
| FCC148 | NGC 1375 | S0 | 19.9 | 10 | 26.9 | 56.0 | 13.5 |
| FCC170 | NGC 1381 | S0 | 21.9 | 10.6 | 12.9 | 153.0 | 12.9 |
| FCC177 | NGC 1380A | S0 | 20.9 | 9.7 | 12.6 | 55.0 | 13.6 |
| FCC277 | NGC 1428 | E5 | 20.7 | 9.9 | 10.1 | 81.7 | 14.1 |
| FCC310 | NGC 1460 | SB0 | 19.9 | 10 | 25.8 | 60.4 | 13.7 |
Notes. Column (1) lists the Ferguson (1989) catalogue designation and (2) the galaxies common names. Column (3) give the galaxies morphological type as listed in Ferguson (1989). The distances (4) are taken from Blakeslee et al. (2009) and are based on surface brightness fluctuations. The dynamical masses (5) are estimated using 
(Cappellari et al. 2006). Reff (6) is taken from Ferguson (1989). The central velocity dispersions (7) are taken from Kuntschner (2000), except for FCC277 and FCC310, which they are taken from Wegner et al. (2003). In order to use these central velocity dispersions as mass estimators in (5) we corrected these using the aperture corrections presented in Falcón-Barroso et al. (2017). Column (8) lists the total B-band magnitude extracted from HyperLeda.
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