Table 1.
Selected properties of VCC 1964 and its associated H I detection (see text for details).
| Property | Value(error) |
|---|---|
| R.A. [J2000] | 12:43:17.83(0.7s) |
| Dec. [J2000] | +08:54:53.00(11) |
| Velocityhel | 1,429(2) km s−1 |
| Distance | 17 Mpc |
| W50, W20 | 26(2), 41(3) km s−1 |
| H I flux | 0.307(0.054) Jy km s−1 |
| MH I | 2.1(0.4)×107 M⊙ |
| mg, mi | 17.61(0.13), 17.27(0.11) |
| Mg, Mi | –13.60(0.13), –13.92(0.11) |
| M* | 2.0×107 M⊙ |
| Re | 17.06(0.41)″ |
| Re | 1.41(0.03) kpc |
| μg | 24.62(0.01) mag arcsec−2 |
| Inclination | 61(0.7) ° |
| Vrot | 14.9(1.6) km s−1 |
| Mbar | 4.8×107 M⊙ |
Notes. We list no estimated uncertainties for the stellar or baryonic mass because they would be formally much lower than the systematics. For example, different stellar mass recipes give results that differ by a factor of a few (see Section 3.4.2), even when the same wavebands are used.
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