Table 4.
Estimates of the mass (in units of M⊙) and age (in Myr) for different choices of the rotational velocity distribution.
| Star | Teff | log L | ve sin i | H08 |
Flat |
VFTS |
|||
|---|---|---|---|---|---|---|---|---|---|
| Mass | Age | Mass | Age | Mass | Age | ||||
| 0099 | 18 000 | 3.79 | 98 | 7.0 | 36.8 | 7.0 | 36.8 | 7.0 | 36.8 |
| 0070 | 30 500 | 4.43 | 102 | 13.8 | 7.9 | 13.8 | 7.8 | 13.8 | 7.7 |
| 1088 | 19 850 | 4.06 | 184 | 8.6 | 24.7 | 8.8 | 24.7 | 8.6 | 24.7 |
| 1230 | 29 650 | 4.06 | 198 | 11.8 | 3.9 | 11.8 | 3.4 | 11.8 | 3.5 |
| 1212 | 21 500 | 3.78 | 307 | 8.0 | 24.0 | 8.0 | 24.0 | 8.0 | 24.0 |
| 0079 | 29 500 | 4.37 | 308 | 13.4 | 8.0 | 13.4 | 7.8 | 13.4 | 7.9 |
Notes. Estimates are provided for the adopted distribution of Hunter et al. (2008a) (H08), a flat distribution (Flat) and the distribution found by Dufton et al. (2013) for B-type stars in 30 Doradus (30 Dor) and are given to one decimal place to aid comparisons. Other stellar parameters are taken from Table A.2.
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