Table A.3
Properties of binary stellar models for an initial primary mass of 15 M⊙, conservative mass transfer and with variation of the initial secondary mass M2i and initial orbital period Porb.
| No. | M2i | M1f | M2f | Porb | MH1 | log |
T eff, 1 | log |
Teff, 2 | ∗ 1/ ∗ 2 | ≠ Time |
| (M⊙) | (M⊙) | (M⊙) | (Days) | (M⊙) | (103 K) | (103 K) | (yr) | ||||
|
|
|||||||||||
| g2a | 14.94 | 5.60 | 22.26 | 1200 | 0.2178 | 5.06 | 3.66 | 5.08 | 3.63 | *2 | 14 200 |
| g2b | 14.99 | 5.61 | 21.75 | 1200 | 0.2211 | 5.06 | 3.66 | 5.08 | 3.63 | *2 | 70 400 |
| g3a | 14.74 | 5.62 | 22.01 | 1300 | 0.2061 | 5.07 | 3.60 | 4.90 | 3.79 | *1 | / |
| g3b | 14.75 | 5.62 | 22.02 | 1300 | 0.2058 | 5.07 | 3.60 | 4.90 | 3.79 | *1 | / |
| g3c | 14.93 | 5.64 | 22.18 | 1300 | 0.2036 | 5.07 | 3.59 | 5.02 | 3.67 | *1 | / |
| g3d | 14.94 | 5.76 | 22.18 | 1300 | 0.2638 | 5.07 | 3.59 | 5.07 | 3.64 | *2 | 300 |
| g3e | 14.99 | 5.80 | 21.37 | 1300 | 0.2894 | 5.07 | 3.58 | 5.08 | 3.62 | *2 | 63 100 |
| g4a | 14.55 | 5.79 | 21.64 | 1400 | 0.2761 | 5.07 | 3.53 | 4.86 | 3.83 | *1 | / |
| g4b | 14.9 | 5.84 | 21.94 | 1400 | 0.3081 | 5.07 | 3.51 | 4.95 | 3.74 | *1 | / |
| g4c | 14.94 | 5.84 | 21.98 | 1400 | 0.3087 | 5.07 | 3.51 | 5.04 | 3.66 | *1 | / |
| g4d | 14.95 | 6.02 | 21.79 | 1400 | 0.4012 | 5.07 | 3.51 | 5.07 | 3.63 | *2 | 7900 |
| g4e | 14.99 | 6.03 | 21.01 | 1400 | 0.4012 | 5.07 | 3.51 | 5.08 | 3.61 | *2 | 58 300 |
| g5a | 14.37 | 5.98 | 21.24 | 1500 | 0.3656 | 5.07 | 3.47 | 4.81 | 3.85 | *1 | / |
| g5b | 14.4 | 5.99 | 21.27 | 1500 | 0.3728 | 5.07 | 3.47 | 4.82 | 3.85 | *1 | / |
| g5c | 14.55 | 6.01 | 21.40 | 1500 | 0.3904 | 5.07 | 3.45 | 4.85 | 3.82 | *1 | / |
| g5d | 14.9 | 6.06 | 21.69 | 1500 | 0.4240 | 5.07 | 3.45 | 4.95 | 3.74 | *1 | / |
| g5e | 14.94 | 6.06 | 21.73 | 1500 | 0.4244 | 5.07 | 3.45 | 5.04 | 3.66 | *1 | / |
| g5f | 14.95 | 6.27 | 21.56 | 1500 | 0.5305 | 5.07 | 3.45 | 5.07 | 3.63 | *2 | 9100 |
| g5g | 14.99 | 6.28 | 20.56 | 1500 | 0.5328 | 5.07 | 3.45 | 5.07 | 3.60 | *2 | 59 500 |
| g6a | 14.18 | 6.20 | 20.81 | 1600 | 0.4796 | 5.07 | 3.42 | 4.78 | 3.88 | *1 | / |
| g6b | 14.2 | 6.20 | 20.83 | 1600 | 0.4980 | 5.07 | 3.42 | 4.77 | 3.88 | *1 | / |
| g6c | 14.3 | 6.22 | 20.91 | 1600 | 0.4997 | 5.07 | 3.42 | 4.80 | 3.86 | *1 | / |
| g6d | 14.4 | 6.23 | 20.99 | 1600 | 0.5236 | 5.07 | 3.42 | 4.82 | 3.85 | *1 | / |
Notes. The secondary is, for every model, at the start of mass transfer on the giant branch. The column with *1/*2 indicates which star in the binary system explodes first. The time difference between the two stars reaching carbon burning is indicated if star 2 explodes before star 1. The other symbols have a similar meaning as in Table A.1.
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