Table 9
Estimates of the stellar parameters obtained from different single-star evolutionary grids.
| Star | ST | Grid | v o | Me | Mo | log t | ||
|
|
||||||||
| 270 | B3 1b | B11 | 0 | 12 | 12 | 7.21 | ||
| B11 | 225 | 12 | 13 | 7.18 | ||||
| B11 | 400 | 12 | 12 | 7.23 | ||||
| E12Z002 | 0 | 12 | 13 | 7.14 | ||||
| E12Z014 | 0 | 14 | 14 | 7.09 | ||||
| E12Z002 | 260 | 12 | 12 | 7.28 | ||||
| E12Z014 | 260 | 12 | 12 | 7.24 | ||||
|
|
||||||||
| 261 | B5 Ia | B11 | 0 | 20 | 20 | 6.91 | ||
| B11 | 225 | 20 | 20 | 6.91 | ||||
| B11 | 400 | 19 | 20 | 6.94 | ||||
| E12Z002 | 0 | 18 | 18 | 6.99 | ||||
| E12Z014 | 0 | 19 | 20 | 6.90 | ||||
| E12Z002 | 260 | 15 | 15 | 7.16 | ||||
| E12Z014 | 260 | 18 | 18 | 7.03 | ||||
|
|
||||||||
| 578 | B1.5 Ia | B11 | 0 | 26 | 27 | 6.79 | ||
| B11 | 225 | 26 | 27 | 6.78 | ||||
| B11 | 400 | 24 | 25 | 6.86 | ||||
| E12Z002 | 0 | 26 | 26 | 6.80 | ||||
| E12Z014 | 0 | 28 | 29 | 6.75 | ||||
| E12Z002 | 260 | 24 | 24 | 6.90 | ||||
| E12Z014 | 260 | 23 | 24 | 6.92 | ||||
|
|
||||||||
| 590 | B0.7 Iab | B11 | 0 | 39 | 42 | 6.60 | ||
| B11 | 225 | 36 | 39 | 6.63 | ||||
| B11 | 400 | 30 | 33 | 6.76 | ||||
| E12Z002 | 0 | 35 | 36 | 6.69 | ||||
| E12Z014 | 0 | 36 | 40 | 6.65 | ||||
| E12Z002 | 260 | 30 | 31 | 6.82 | ||||
| E12Z014 | 260 | 26 | 29 | 6.86 | ||||
|
|
||||||||
| 003 | B1 Ia+ | B11 | 0 | 46 | 50 | 6.55 | ||
| B11 | 225 | 44 | 49 | 6.56 | ||||
| B11 | 400 | 30 | 33 | 6.76 | ||||
| E12Z002 | 0 | 38 | 39 | 6.67 | ||||
| E12Z014 | 0 | 50: | 57: | 6.55 | ||||
| E12Z002 | 260 | 35 | 36 | 6.77 | ||||
| E12Z014 | 260 | 28 | 32 | 6.83 | ||||
Notes. B11 is from the grid of Brott et al. (2011) for an LMC metallicity. E12Z014 is from Ekström et al. (2012) for Galactic metallicity, with E12Z002 being for a lower (near SMC) metallicity. The rotating models of Ekström et al. (2012) are for an intital rotational velocity of 40% of the critical value that translates to vo~ 260 km s-1. Masses are in units of the solar mass and time is in years.
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