Table 8.
Comparison between the predicted turn-off masses for given ages in various stellar models.
| Age (Myr) | MTO (M⊙) Bressan et al. non-rotating |
MTO (M⊙) Ekström et al. non-rotating |
MTO (M⊙) Ekström et al. with rotation |
|---|---|---|---|
| 80 | 5.6 | 5.4 | 6.0 |
| 160 | 4.2 | 4.0 | 4.4 |
| 250 | 3.5 | 3.4 | 3.7 |
| 280 | 3.4 | 3.4 | 3.7 |
| 350 | 3.1 | 3.0 | 3.4 |
| 400 | 3.0 | 2.8 | 3.0 |
| 430 | 2.9 | 2.8 | 3.0 |
| 500 | 2.7 | 2.6 | 2.8 |
| 610 | 2.5 | 2.6 | 2.4 |
Notes. The Bressan et al. (2012) isochrones were computed for the exact age using the PARSEC on-line interface (http://stev.oapd.inaf.it/cgi-bin/cmd). The isochrones from Ekström et al. (2012) are available at steps of 0.1 dex in log(Age). We list the turn-off values for these pre-computed isochrones with age closest to the age listed in the first column of the table.
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