Table 2.
Stellar parameters for models at different evolutionary stages.
| Xc/Xini | Model | log L (L⊙) | R (R⊙) | Age (Myr) | Mcc (M⊙) | Π0 (s) |
|---|---|---|---|---|---|---|
| standard | 2.713 | 2.583 | 8.44 | 1.225 | 10777.6 | |
| 0.9 | standard+rot | 2.710 | 2.606 | 8.51 | 1.223 | 10721.0 |
| standard+rot+R-MLT | 2.709 | 2.606 | 8.19 | 1.225 | 10700.3 | |
| standard | 2.896 | 3.749 | 75.10 | 0.903 | 10632.6 | |
| 0.5 | standard+rot | 2.893 | 3.795 | 75.38 | 0.901 | 10588.0 |
| standard+rot+R-MLT | 2.881 | 3.741 | 72.29 | 0.887 | 10478.2 | |
| standard | 3.055 | 6.518 | 110.03 | 0.525 | 8228.8 | |
| 0.1 | standard+rot | 3.052 | 6.607 | 110.45 | 0.525 | 8196.9 |
| standard+rot+R-MLT | 3.027 | 6.239 | 106.44 | 0.509 | 8040.3 | |
Notes. The listed quantities are stellar luminosity (log L), stellar radius (R), age, convective core mass (Mcc), and buoyancy travel time (Π0). The three evolutionary stages correspond to models near the ZAMS (Xc/Xini = 0.9), mid–main sequence (Xc/Xini = 0.5), and near the TAMS (Xc/Xini = 0.1). The evolutionary stage is indicated by the central hydrogen mass fraction Xc/Xini.
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