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Table C.1.
How most stellar parameters remain similar throughout the stripped phase.
| XHe, c | Age (a) | Mstrip(a) | R⋆(a) | Reff(b) | T⋆(a) | Teff(b) | log10g⋆(a) | log10geff(b) | log10L(a) | log10 Ṁwind(a) | XH, s(a) | XHe, s(a) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [Myr] | [M⊙] | [R⊙] | [R⊙] | [kK] | [kK] | [cm s−2] | [cm s−2] | [L⊙] | [M⊙ yr−1] | |||
| Minit = 8.15 M⊙ | ||||||||||||
| 0.9 | 37.3 | 2.22 | 0.67 | 0.67 | 61.1 | 61.0 | 5.13 | 5.13 | 3.75 | −7.3 | 0.24 | 0.746 |
| 0.8 | 37.6 | 2.21 | 0.55 | 0.55 | 61.2 | 61.1 | 5.3 | 5.3 | 3.58 | −7.53 | 0.245 | 0.741 |
| 0.7 | 37.9 | 2.2 | 0.54 | 0.54 | 61.2 | 61.1 | 5.31 | 5.31 | 3.57 | −7.55 | 0.243 | 0.743 |
| 0.6 | 38.2 | 2.19 | 0.54 | 0.54 | 61.4 | 61.3 | 5.31 | 5.31 | 3.57 | −7.54 | 0.239 | 0.747 |
| 0.5 | 38.5 | 2.18 | 0.55 | 0.55 | 61.7 | 61.6 | 5.3 | 5.3 | 3.59 | −7.52 | 0.238 | 0.748 |
| 0.4 | 38.8 | 2.17 | 0.55 | 0.55 | 62.2 | 62.0 | 5.3 | 5.29 | 3.61 | −7.47 | 0.219 | 0.767 |
| 0.3 | 39.1 | 2.16 | 0.55 | 0.55 | 62.9 | 62.8 | 5.29 | 5.29 | 3.63 | −7.45 | 0.22 | 0.766 |
| 0.2 | 39.4 | 2.15 | 0.54 | 0.55 | 64.2 | 64.0 | 5.3 | 5.3 | 3.65 | −7.4 | 0.212 | 0.774 |
| 0.1 | 39.7 | 2.14 | 0.52 | 0.52 | 66.4 | 66.4 | 5.33 | 5.33 | 3.68 | −7.37 | 0.21 | 0.776 |
| Minit = 12.17 M⊙ | ||||||||||||
| 0.9 | 18.8 | 3.99 | 1.24 | 1.25 | 69.1 | 68.8 | 4.85 | 4.84 | 4.5 | −6.34 | 0.247 | 0.739 |
| 0.8 | 18.9 | 3.95 | 0.81 | 0.82 | 75.8 | 75.6 | 5.21 | 5.21 | 4.29 | −6.6 | 0.236 | 0.75 |
| 0.7 | 19.1 | 3.92 | 0.77 | 0.78 | 76.7 | 76.5 | 5.26 | 5.25 | 4.27 | −6.63 | 0.226 | 0.76 |
| 0.6 | 19.2 | 3.9 | 0.76 | 0.76 | 77.5 | 77.3 | 5.27 | 5.26 | 4.27 | −6.62 | 0.218 | 0.768 |
| 0.5 | 19.3 | 3.86 | 0.75 | 0.76 | 78.5 | 78.3 | 5.27 | 5.27 | 4.29 | −6.59 | 0.213 | 0.773 |
| 0.4 | 19.4 | 3.83 | 0.74 | 0.74 | 80.1 | 80.0 | 5.29 | 5.28 | 4.3 | −6.56 | 0.201 | 0.785 |
| 0.3 | 19.5 | 3.8 | 0.7 | 0.7 | 82.8 | 82.7 | 5.32 | 5.32 | 4.32 | −6.52 | 0.179 | 0.807 |
| 0.2 | 19.7 | 3.75 | 0.63 | 0.63 | 88.1 | 87.9 | 5.41 | 5.41 | 4.34 | −6.44 | 0.106 | 0.88 |
| 0.1 | 19.8 | 3.68 | 0.57 | 0.57 | 93.5 | 93.4 | 5.49 | 5.49 | 4.35 | −6.33 | 7.735 × 10−4 | 0.986 |
| Minit = 18.17 M⊙ | ||||||||||||
| 0.9 | 10.7 | 7.16 | 1.99 | 2.02 | 74.4 | 73.9 | 4.69 | 4.68 | 5.04 | −5.63 | 0.232 | 0.755 |
| 0.8 | 10.7 | 7.04 | 1.11 | 1.11 | 90.7 | 90.4 | 5.2 | 5.19 | 4.87 | −5.83 | 0.213 | 0.774 |
| 0.7 | 10.8 | 6.95 | 1.02 | 1.03 | 93.4 | 93.2 | 5.26 | 5.25 | 4.86 | −5.84 | 0.195 | 0.791 |
| 0.6 | 10.9 | 6.85 | 0.97 | 0.97 | 96.2 | 95.9 | 5.3 | 5.29 | 4.86 | −5.82 | 0.176 | 0.811 |
| 0.5 | 10.9 | 6.74 | 0.88 | 0.88 | 101.6 | 101.3 | 5.38 | 5.38 | 4.87 | −5.76 | 0.117 | 0.87 |
| 0.4 | 11.0 | 6.61 | 0.79 | – | 107.1 | – | 5.46 | – | 4.87 | −5.66 | 1.12 × 10−3 | 0.985 |
| 0.3 | 11.1 | 6.44 | 0.79 | 0.8 | 107.2 | 106.5 | 5.45 | 5.44 | 4.87 | −5.66 | 3.556 × 10−9 | 0.986 |
| 0.2 | 11.1 | 6.27 | 0.78 | 0.79 | 107.8 | 107.0 | 5.45 | 5.43 | 4.87 | −5.66 | 4.273 × 10−15 | 0.986 |
| 0.1 | 11.2 | 6.07 | 0.76 | 0.77 | 109.4 | 108.6 | 5.46 | 5.44 | 4.87 | −5.66 | 8.791 × 10−18 | 0.986 |
Notes. Here, we show three example models with initial masses of Minit = 8.2, 12.2, and 18.2 M⊙ that are stripped as they fill their Roche-lobes during the Hertzsprung gap evolution. The models have solar metallicity.
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