Table 1.
Relevant properties of the three galaxies FCC 153 and FCC 177, analyzed here, and FCC 170, analyzed in Paper I.
| FCC (1) | Alternative | D(2) |  |
 |
 |
M |
 |
 |
||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| name | names | (Mpc) | (°) | (Mpc) | (″) | (kpc) | (km s−1) | (109 M⊙) | (″) | (kpc) | (″) | (kpc) |
| 153 | IC 1963 | 20.8 | 1.17 | 0.45 | 11.4 | 1.15 | 165 | 7.6 | 5.1 | 0.5 | 0.2 | 0.02 |
| IC 0335 | ||||||||||||
| 177 | NGC 1380A | 20.0 | 0.79 | 0.30 | 15.0 | 1.45 | 120 | 8.5 | 8.4 | 0.8 | 0.4 | 0.04 |
| PGC 13335 | ||||||||||||
| 170 | NGC 1381 | 21.9 | 0.42 | 0.16 | 13.8 | 1.47 | 280 | 22.5 | 10.8 | 1.1 | ||
| PGC 13321 | ||||||||||||
Notes. (1) Galaxy name from the Fornax Cluster Catalog (Ferguson 1989a). (2) Distance from Blakeslee et al. (2009). (3) Projected distance from the cluster central galaxy FCC 213 (Iodice et al. 2019). (4) Effective radius in the B band (Ferguson 1989b). (5) Maximum circular velocity, from Bedregal et al. (2006). (6) Stellar mass as estimated from the i band (Iodice et al. 2019). (7) Lower limit of the region where the thick disk dominates, according to the photometrical decomposition by Comerón et al. (2018). (8) Mean radius of the region dominated by the NSC (from Fig. 3 in Turner et al. 2012).
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