Table 1.
Parameters of the Leo A galaxy.
| Parameter | Value | Reference |
|---|---|---|
| α(J2000); δ(J2000) | 9:59:24.0; +30:44:47 | Vansevičius et al. (2004), RGB stars |
| b/a; PA | 0.60; 114° | Vansevičius et al. (2004), RGB stars |
| (m − M)0 | 24.51 ± 0.12 (0.80 ± 0.04 Mpc) | Dolphin et al. (2002), RR Lyrae stars |
| A(F475W); A(F814W) | 0.068; 0.032 | Schlafly & Finkbeiner (2011) |
| MSTARS | 3.3 × 106 M⊙ | Kirby et al. (2017) |
| MH I | 6.9 × 106 M⊙ | Hunter et al. (2012) |
| M/LV | 20 ± 6 M⊙/L⊙ | Brown et al. (2007), B supergiants and H II zones |
| 12+log(O/H) | 7.38 ± 0.1 | van Zee et al. (2006), a planetary nebula and H II zones |
| 12+log(O/H) | 7.4 ± 0.2 | Ruiz-Escobedo et al. (2018), H II zones |
| <[Fe/H]> |  |
Kirby et al. (2017), RGB stars |
Notes. α(J2000) and δ(J2000) are the equatorial coordinates of the galaxy centre; b/a is the ratio of minor to major axes; PA is the position angle of the major axis; (m − M)0 is the true distance modulus; A(F475W) and A(F814W) are the foreground extinction in corresponding passbands; MSTARS is the stellar mass; MH I is the mass of neutral hydrogen; M/LV is the lower limit of the mass-to-luminosity ratio; 12 + log(O/H) is the oxygen abundance; and <[Fe/H]> is the average metallicity.
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