Table 1.
Parameters adopted from the literature.
| Galaxy | D | r1/2 | rt | MV | M★ | Mgas | N★ | References |
|---|---|---|---|---|---|---|---|---|
| (kpc) | (pc) | (pc) | (mag) | (106 M⊙) | (106 M⊙) | |||
| Carina | 106 ± 6 | 250 ± 39 | 2387 | −9.1 | 0.38 | – | 767 | 1, 2 |
| Fornax | 138 ± 8 | 710 ± 77 | 6083 | −13.4 | 43 | – | 2573 | 3, 2 |
| Draco | 76 ± 6 | 221 ± 19 | 2172 | −8.8 | 0.29 | – | 504 | 4, 5 |
| Leo I | 254 ± 15 | 251 ± 27 | 5299 | −12.0 | 5.5 | – | 328 | 6, 2 |
| Leo II | 233 ± 14 | 176 ± 42 | 3875 | −9.8 | 0.74 | – | 186 | 7, 2 |
| Sculptor | 86 ± 6 | 283 ± 45 | 2502 | −11.1 | 2.3 | – | 1351 | 8, 2 |
| Sextans | 86 ± 4 | 695 ± 44 | 2930 | −9.3 | 0.44 | – | 417 | 9, 2 |
| Ursa Minor | 76 ± 3 | 181 ± 27 | 2279 | −8.8 | 0.29 | – | 430 | 10, 2 |
| Antlia B | 1350 ± 60 | 273 ± 29 | 7777* | −9.7 | 0.76 | 0.28 | 127 | 11, 12, 13 |
| Eridanus II | 366 ± 17 | 277 ± 14 | 5154 | −7.1 | 0.09 | – | 92 | 14, 15 |
| Grus 1 | 125 |  |
1076 | −4.1 | 0.01 | – | 14 | 16, 17, 13 |
| Leo T | 409 ± 28 | 115 ± 17 | 5639 | −7.6 | 0.14 | 0.41 | 75 | 18, 19, 13 |
Notes. From left to right, the columns show the name of the galaxy and galactocentric distance (D⊙); half-light radius (r1/2); tidal radius (rt) estimated with the dynamical masses from Pace (2025); absolute V-band magnitude (MV); stellar mass (M★); gas mass (Mgas); and number of kinematic member stars (N★). The units for each column are marked in the second row. *Obtained using the distance from Ant B to its host D = 72 kpc (Sand et al. 2015) and MNGC3109 = 1.1 × 1010 M⊙ (Huchtmeier 1973). References. (1) Pietrzynski et al. (2009), (2) Irwin & Hatzidimitriou (1995), (3) de Boer et al. (2012), (4) Bonanos et al. (2004), (5) Martin et al. (2008), (6) Bellazzini et al. (2004), (7) Bellazzini et al. (2005), (8) Pietrzynski et al. (2008), (9) Lee et al. (2009), (10) Carrera et al. (2002), (11) Sand et al. (2015), (12) Hargis et al. (2020), (13) Zoutendijk et al. (2021b), (14) Crnojevic et al. (2016), (15) Zoutendijk et al. (2021a), (16) Koposov et al. (2015), (17) Chiti et al. (2022), (18) Clementini et al. (2012), and (19) Wolf et al. (2010).
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