Table 1.
Properties of the target dwarf galaxies in this paper.
| Galaxy | RA, Dec | D | log |
12 + log(O/H) | log |
log |
Θ |
|---|---|---|---|---|---|---|---|
| (J2000) | (Mpc) | (pc) | |||||
| J0921 | 09:21:27.2, +7:21:50.7 | 21 ± 4 (a) | −1.64 ± 0.10 (b) | 7.67 ± 0.20 (c) | 8.44 ± 0.10 (d) | 8.03 ± 0.22 (b) | 83 |
| KKH046 | 09:08:36.2, +5:17:45.5 | 12 ± 2 (a) | −2.37 ± 0.10 (b) | 7.68 ± 0.03 (e) | 7.74 ± 0.23 (a) | 7.09 ± 0.20 (b) | 32 |
| Leo P | 10:21:45.1, +18:05:17.0 | 1.6 ± 0.1 (f) | −4.40 ± 0.38 (b) | 7.17 ± 0.04 (f) | 5.96 ± 0.10 (f) | 5.75 ± 0.30 (f) | 9.8 |
Notes. Columns are (2) their J2000 coordinates, (3) the distance to the galaxy in megaparsecs, (4) their star formation rate (SFR), (5) their oxygen abundance as derived from the direct method, (6) the log of their HI mass in solar mass units, (7) the log of their stellar mass in solar mass units, and (8) the spatial resolution of the MUSE observations.
References. Values are taken from (a)Kourkchi et al. (2020), (b)Marasco et al. (2023), (c)James et al. (2015), (d)Haynes et al. (2018), (e)Izotov et al. (2012), and (f)McQuinn (2015).
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