Table 3.
Properties of NGC 1140 and other BCD galaxies resulting from dwarf-dwarf mergers from Zhang et al. (2020a) and Chhatkuli et al. (2023).
| Galaxy | log M*/M⊙ | log Mgas/M⊙ | log SFR/(M⊙/yr) | log(Rs, inner)/kpc.h−1 | μ0, B(inner) |
|---|---|---|---|---|---|
| NGC 1140 | 8.98 | 9.34 | 0.63 | –0.23 | 20.04 |
| VCC 848 | 8.32 | 8.62 | –1.60 | –0.32 | 20.52 |
| D004 | 9.09 | 8.43 | –1.08 | –0.44 | 19.67 |
| D036 | 8.56 | 8.87 | – | –0.38 | 20.68 |
| D047 | 8.26 | – | –1.46 | –0.8 | 19.16 |
| D055 | 9.18 | 8.19 | –0.85 | –0.15 | 20.21 |
| D075 | 9.03 | 9.94 | –0.68 | –0.45 | 19.93 |
| D076 | 7.92 | 8.40 | – | –0.007 | 20.549 |
Notes. For the stellar mass, SFR, and gas mass, we report values from the literature except for NGC 1140 for which we use the results of the SED fitting (le Phare, Section 3.4). For Rs, inner and μ0, B(inner), we fitted the profiles provided by the authors to compare to ours. The log SFR has been converted from Kennicutt (1998) to Kroupa (2001) using the conversion of Argence & Lamareille (2009).
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