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Table 2.
Final properties of the stars in this study.
| Ṁ | End-point | tH | tred/ttot | Mfinal | Xc, final | Mcore |
|---|---|---|---|---|---|---|
| M⊙ yr−1 | Myr | M⊙ | M⊙ | |||
| 0.000001 | End Si-burn | 22.5 | 0.002 | 22.5 | 0 | 5.2 |
| 0.00001 | End Si-burn | 8.40 | 0.002 | 86 | 0 | 13 |
| 0.0001 | End Si-burn | 4.36 | 0.002 | 436 | 0 | 121 |
| 0.001 | End Si-burn | 2.796 | 0.003 | 3053 | 0 | 660 |
| 0.010 | Mid He-burn (0.49Yc) | 2.261 | 0.998 | 22 600 | 0 | 9912 |
| 0.050 | GR instab. (0.99Yc) | 1.680 | 0.903 | 80 206 | 0 | 44 792 |
| 0.075 | GR instab. | 1.345 | 0.826 | 100 972 | 0.16 | 62 017 |
| 0.1 | GR instab. | 1.040 | 0.630 | 108 000 | 0.244 | 67 330 |
| 1 | GR instab. | 0.214 | 0.230 | 214 100 | 0.525 | 60 090 |
| 10 | GR instab. | 0.045 | 0.438 | 449 700 | 0.619 | 47 560 |
| 100 | GR instab. | 0.007 | 0.194 | 697 200 | 0.721 | 7406 |
| 1000 | GR instab. | 0.001 | 0.118 | 1 027 570 | 0.751 | 0 |
Notes. Xc, final is the core H mass fraction at the end of the life of the star. Mcore represents the mass of the convective core.
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