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Table D.1.
Effect of a modified wind mass loss factor after mass transfer on the stellar properties of binary-stripped stars
| Wind factor | M* | log10 | log10 | log10 |
|---|---|---|---|---|
| (M⊙) | (Teff/K) | (L/L⊙) | (Ṁ/[M⊙ yr−1]) | |
| Binary-stripped star model:Mi = 11 M⊙ | ||||
| 0.10 | 3.50 | 4.84 | 4.19 | -7.79 |
| 0.33 | 3.46 | 4.85 | 4.17 | -7.28 |
| 0.50 | 3.43 | 4.85 | 4.15 | -7.11 |
| 0.75 | 3.39 | 4.86 | 4.14 | -6.94 |
| 1.00 | 3.36 | 4.86 | 4.12 | -6.82 |
| 1.25 | 3.32 | 4.87 | 4.11 | -6.73 |
| 2.00 | 3.22 | 4.89 | 4.08 | -6.52 |
| 3.00 | 3.08 | 4.92 | 4.03 | -6.27 |
| Binary-stripped star model:Mi = 20 M⊙ | ||||
| 0.10 | 8.10 | 4.92 | 5.04 | -6.68 |
| 0.33 | 7.94 | 4.95 | 5.02 | -6.17 |
| 0.50 | 7.84 | 4.97 | 5.00 | -5.98 |
| 0.75 | 7.68 | 4.99 | 4.99 | -5.80 |
| 1.00 | 7.52 | 5.02 | 4.97 | -5.62 |
| 1.25 | 7.34 | 5.04 | 4.95 | -5.46 |
| 2.00 | 6.81 | 5.03 | 4.88 | -5.34 |
| 3.00 | 6.22 | 5.02 | 4.80 | -5.27 |
Notes. The values are taken halfway through central helium burning (defined as the moment when XHe = 0.5).
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