Table 2
Stellar masses, Hi masses, dust masses, star formation rates, metallicities, Hi deficiency, and adopted distances of star-forming dwarf galaxies detected by HeViCS.
| ID | log (M⋆) | log (MHI) | log (Md)† | log (SFR) | 12 + log (O/H) | 12 + log (O/H) | DefHI | D |
| [ M⊙ ] | [ M⊙] | [ M⊙] | [ M⊙ yr-1] | PT05 | [Mpc] | |||
|
|
||||||||
| VCC1 | 8.94 ± 0.04 | 7.50 ± 0.10 | 5.25 |
–1.35 ± 0.08a | 8.59 ± 0.10 | – | 1.20 | 32.0 |
| VCC10 | 8.95 ± 0.04 | 8.74 ± 0.01 | 6.13 |
–1.05 ± 0.08a | 8.56 ± 0.10 | – | 0.10 | 32.0 |
| VCC17 | 8.42 ± 0.04 | 8.90 ± 0.01 | 5.86 ∗ |
–0.95 ± 0.09b | 8.59 ± 0.10 | – | –0.13 | 32.0 |
| VCC22 | 8.43 ± 0.04 | 8.21 ± 0.03 | 5.44∗ |
–1.93 ± 0.22c | – | – | –0.16 | 32.0 |
| VCC24 | 8.83 ± 0.04 | 8.98 ± 0.01 | 5.59 |
–1.88 ± 0.22c | 8.31 ± 0.10 | – | –0.15 | 32.0 |
| VCC87 | 8.39 ± 0.04 | 8.51 ± 0.01 | 5.91 |
–1.62 ± 0.07a | 8.25 ± 0.10 | – | 0.17 | 17.0 |
| VCC135 | 9.44 ± 0.04 | 7.19 ± 0.08 | 6.19 |
–1.03 ± 0.08a | 8.65 ± 0.10 | 8.47 | 1.73 | 32.0 |
| VCC144 | 8.81 ± 0.05 | 8.76 ± 0.01 | 5.70 |
–0.27 ± 0.05a | 8.21 ± 0.10 | 8.30 | –0.21 | 32.0 |
| VCC172 | 8.88 ± 0.04 | 8.95 ± 0.01 | 6.04 |
–1.45 ± 0.09b | 8.58 ± 0.10 | – | 0.01 | 32.0 |
| VCC213 | 8.89 ± 0.04 | 7.84 ± 0.03 | 5.84 |
–1.20 ± 0.06a | 8.77 ± 0.12 | 8.27 | 0.57 | 17.0 |
| VCC223 | 8.45 ± 0.04 | 7.79 ± 0.07 | 5.61 |
–1.33 ± 0.07a | 8.20 ± 0.10 | – | 0.40 | 32.0 |
| VCC281 | 8.15 ± 0.04 | 7.51 ± 0.04 | 5.32 |
–2.05 ± 0.22c | 8.49 ± 0.10 | – | 0.33 | 17.0 |
| VCC286 | 8.26 ± 0.04 | <7.93 | 5.35∗ |
–2.00 ± 0.22c | 8.46 ± 0.10 | – | >0.50 | 32.0 |
| VCC322 | 8.00 ± 0.04 | 8.27 ± 0.01 | 4.93 |
–2.29 ± 0.25c | 8.58 ± 0.10 | – | 0.31 | 17.0 |
| VCC324 | 8.72 ± 0.04 | 8.23 ± 0.01 | 5.50 |
–0.75 ± 0.07a | 8.14 ± 0.10 | 8.37 | 0.40 | 17.0 |
| VCC328 | 7.66 ± 0.04 | 7.99 ± 0.01 | 4.70 |
–2.33 ± 0.25c | 8.46 ± 0.10 | – | 0.46 | 17.0 |
| VCC334 | 8.04 ± 0.04 | 7.95 ± 0.01 | 4.94 |
–1.77 ± 0.17c | 8.22 ± 0.10 | 7.92 | 0.17 | 17.0 |
| VCC340 | 9.11 ± 0.04 | 8.89 ± 0.01 | 6.05 |
–0.84 ± 0.07a | 8.26 ± 0.10 | – | –0.01 | 32.0 |
| VCC367 | 8.24 ± 0.04 | <7.99 | 5.64∗ |
– | – | – | >0.50 | 32.0 |
| VCC446 | 8.36 ± 0.04 | 7.79 ± 0.04 | 5.30 |
–1.79 ± 0.17c | 8.25 ± 0.10 | – | 0.75 | 23.0 |
| VCC562 | 7.76 ± 0.04 | 7.74 ± 0.03 | 5.00 |
–1.74 ± 0.17c | 8.10 ± 0.10 | 8.32 | 0.44 | 17.0 |
| VCC620 | 8.00 ± 0.04 | 8.06 ± 0.01 | 5.25 ∗ |
–1.97 ± 0.22c | 8.24 ± 0.10 | – | 0.52 | 17.0 |
| VCC641 | 8.11 ± 0.04 | 7.86 ± 0.04 | 5.45∗ |
–1.83 ± 0.17c | 8.21 ± 0.10 | – | 0.59 | 23.0 |
| VCC693 | 8.33 ± 0.04 | 8.27 ± 0.01 | 5.55 |
–1.93 ± 0.22c | 8.43 ± 0.10 | – | 0.27 | 17.0 |
| VCC699 | 9.19 ± 0.04 | 8.94 ± 0.01 | 6.26 |
–0.63 ± 0.06a | 8.30 ± 0.10 | – | 0.08 | 23.0 |
| VCC737 | 8.35 ± 0.04 | 8.66 ± 0.01 | 5.73 |
–1.85 ± 0.17c | 8.28 ± 0.10 | – | –0.17 | 17.0 |
| VCC741 | 7.82 ± 0.04 | <8.04 | 5.17 |
–2.04 ± 0.22c | 8.54 ± 0.10 | – | >0.31 | 17.0 |
| VCC802 | 7.58 ± 0.04 | <6.70 | 4.97∗ |
–2.02 ± 0.22c | 8.45 ± 0.10 | 8.35 | >1.49 | 17.0 |
| VCC825 | 8.30 ± 0.04 | <7.16 | 4.86∗ |
– | 8.79 ± 0.10 | – | >1.47 | 23.0 |
| VCC841 | 8.12 ± 0.04 | 7.68 ± 0.03 | 5.20 |
–1.62 ± 0.07a | 8.33 ± 0.10 | 8.34 | 0.68 | 17.0 |
| VCC848 | 8.48 ± 0.04 | 8.92 ± 0.01 | 5.30 |
–1.42 ± 0.09b | 8.61 ± 0.10 | 8.12 | –0.20 | 23.0 |
| VCC888 | 8.41 ± 0.04 | 8.41 ± 0.02 | 5.97 |
–2.24 ± 0.25c | – | – | 0.31 | 23.0 |
| VCC985 | 8.00 ± 0.04 | 7.46 ± 0.04 | 4.93 |
–2.07 ± 0.22c | 8.35 ± 0.10 | – | 0.72 | 17.0 |
| VCC1021 | 8.49 ± 0.04 | 7.77 ± 0.05 | 4.87∗ |
–2.46 ± 0.25c | – | – | 0.95 | 23.0 |
| VCC1141 | 8.27 ± 0.04 | 8.12 ± 0.03 | 5.24 |
–2.05 ± 0.22c | 8.32 ± 0.10 | – | 0.05 | 23.0 |
| VCC1179 | 8.34 ± 0.04 | 7.70 ± 0.05 | 5.12 |
–1.66 ± 0.07a | 8.33 ± 0.10 | – | 1.02 | 23.0 |
| VCC1200 | 8.05 ± 0.04 | 8.22 ± 0.01 | 5.13 |
–2.04 ± 0.22c | 8.57 ± 0.10 | – | 0.38 | 17.0 |
| VCC1273 | 8.69 ± 0.04 | <7.16 | 5.36 |
–2.67 ± 0.57c | 8.59 ± 0.10 | – | >1.56 | 23.0 |
| VCC1356 | 8.23 ± 0.04 | 8.38 ± 0.01 | 5.30 |
–1.69 ± 0.06a | 8.34 ± 0.10 | – | 0.14 | 17.0 |
| VCC1374 | 8.46 ± 0.04 | 8.26 ± 0.01 | 5.66 |
–1.40 ± 0.07a | 8.63 ± 0.10 | 8.26 | 0.31 | 17.0 |
| VCC1437 | 8.52 ± 0.04 | 8.03 ± 0.02 | 5.23 |
–1.78 ± 0.17c | 8.38 ± 0.10 | 8.00 | 0.11 | 17.0 |
| VCC1455 | 7.77 ± 0.04 | 7.21 ± 0.07 | 5.02∗ |
–2.24 ± 0.22c | 8.40 ± 0.10 | – | 0.98 | 17.0 |
| VCC1554 | 9.64 ± 0.04 | 9.45 ± 0.01 | 6.81 |
0.11 ± 0.07a | 8.26 ± 0.10 | – | –0.43 | 17.0 |
| VCC1575 | 9.25 ± 0.04 | 7.97 ± 0.02 | 6.24 |
–0.90 ± 0.10a | 8.76 ± 0.10 | – | 0.89 | 17.0 |
| VCC1675 | 8.60 ± 0.04 | 7.44 ± 0.03 | 5.23 |
–2.22 ± 0.25c | 8.45 ± 0.10 | – | 1.15 | 17.0 |
| VCC1686 | 9.07 ± 0.04 | 8.68 ± 0.01 | 6.44 |
–0.89 ± 0.07a | – | – | 0.38 | 17.0 |
| VCC1699 | 8.57 ± 0.04 | 8.77 ± 0.01 | 5.46 |
–1.12 ± 0.08a | 8.07 ± 0.12 | 7.88 | –0.06 | 17.0 |
| VCC1725 | 8.59 ± 0.04 | 8.21 ± 0.01 | 5.78 |
–1.36 ± 0.07a | 8.25 ± 0.10 | 8.31 | 0.50 | 17.0 |
| VCC1791 | 8.52 ± 0.04 | 8.72 ± 0.01 | 5.71 |
–1.08 ± 0.05a | 8.16 ± 0.10 | – | –0.11 | 17.0 |
Notes.
Dust masses were determined fitting a single MBB with a fixed β = 1.5 emissivity from 100 to 350 μm. Galaxies noted with (∗) correspond to MBB fits with fixed dust temperature, because of the lack of enough data points (see also Table 4).
SFR calculated from Eq. (4) (Wen et al. 2014).
SFR calculated from Eq. (5) (Kennicutt & Evans 2012).
SFR calculated from Eq. (6) (Lee et al. 2009).
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