Table B.1.
Initial mass, stripped star mass calculated two ways, main sequence lifetime, and stripped star lifetime for Z = 0.014 models.
Minit (M⊙) | MHe (M⊙)a | Mstrip (M⊙)b | tMS (yr)a | tstrip (yr)b |
---|---|---|---|---|
2.00 | 0.22 | 0.35 | 1.17 × 109 | – |
2.21 | 0.26 | 0.38 | 8.96 × 108 | 4.14 × 108 |
2.44 | 0.29 | 0.44 | 6.84 × 108 | – |
2.70 | 0.33 | 0.51 | 5.22 × 108 | 1.33 × 108 |
2.99 | 0.38 | 0.58 | 4.00 × 108 | – |
3.30 | 0.44 | 0.67 | 3.07 × 108 | 6.39 × 107 |
3.65 | 0.50 | 0.74 | 2.37 × 108 | 4.20 × 107 |
4.04 | 0.57 | 0.85 | 1.84 × 108 | 2.81 × 107 |
4.46 | 0.65 | 0.97 | 1.44 × 108 | 2.00 × 107 |
4.93 | 0.76 | 1.12 | 1.13 × 108 | 1.65 × 107 |
5.45 | 0.88 | 1.28 | 8.94 × 107 | 1.06 × 107 |
6.03 | 1.01 | 1.43 | 7.14 × 107 | 8.04 × 106 |
6.66 | 1.18 | 1.64 | 5.74 × 107 | 6.42 × 106 |
7.37 | 1.38 | 1.89 | 4.66 × 107 | 4.41 × 106 |
8.15 | 1.61 | 2.18 | 3.81 × 107 | 3.40 × 106 |
9.00 | 1.88 | 2.50 | 3.14 × 107 | 2.70 × 106 |
9.95 | 2.20 | 2.88 | 2.62 × 107 | 2.16 × 106 |
11.00 | 2.59 | 3.34 | 2.19 × 107 | 1.74 × 106 |
12.17 | 3.04 | 3.86 | 1.85 × 107 | 1.43 × 106 |
13.45 | 3.58 | 4.46 | 1.58 × 107 | 1.20 × 106 |
14.87 | 4.22 | 5.14 | 1.37 × 107 | 1.03 × 106 |
16.44 | 4.93 | 5.90 | 1.19 × 107 | 8.93 × 105 |
18.17 | 5.73 | 6.74 | 1.05 × 107 | 7.91 × 105 |
20.09 | 6.68 | – | 9.33 × 106 | – |
22.21 | 7.73 | – | 8.34 × 106 | – |
24.55 | 8.91 | – | 7.53 × 106 | – |
27.13 | 10.20 | – | 6.83 × 106 | – |
30.00 | 11.71 | – | 6.25 × 106 | – |
33.16 | 13.37 | – | 5.75 × 106 | – |
36.65 | 15.21 | – | 5.31 × 106 | – |
40.52 | 17.22 | – | 4.94 × 106 | – |
44.79 | 19.51 | – | 4.62 × 106 | – |
49.51 | 22.08 | – | 4.33 × 106 | – |
54.73 | 24.93 | – | 4.08 × 106 | – |
60.50 | 28.00 | – | 3.86 × 106 | – |
66.89 | 31.66 | – | 3.66 × 106 | – |
73.94 | 35.64 | – | 3.48 × 106 | – |
81.74 | 40.02 | – | 3.32 × 106 | – |
90.38 | 44.64 | – | 3.19 × 106 | – |
99.91 | 47.56 | – | 3.06 × 106 | – |
Notes. For each of our MESA models, the initial mass, the mass of the helium core of a single star model at terminal age main sequence, the mass of the stripped star in a binary model when the central helium mass fraction reaches 0.5, the main sequence lifetime, and the stripped star lifetime. The second and third columns are the same values as plotted in Fig. 3.
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