Table A.1
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 |
| (M⊙) | (M⊙) | (M⊙) | (Days) | (M⊙) | (103 K) | (103 K) | |||
|
|
|||||||||
| 0a | 14.99 | 5.20 | 22.88 | 1000 | 0.0997 | 5.04 | 3.75 | 5.17 | 12.7 |
| 0b | 14.95 | 5.19 | 22.85 | 1000 | 0.0992 | 5.04 | 3.76 | 5.17 | 13.6 |
| 0c | 14.9 | 5.19 | 22.80 | 1000 | 0.0982 | 5.04 | 3.76 | 5.16 | 13.8 |
| 0d | 14.87 | 5.19 | 22.78 | 1000 | 0.0982 | 5.04 | 3.76 | 5.16 | 15.3 |
| 0e | 14.86 | 5.19 | 22.77 | 1000 | 0.0981 | 5.04 | 3.76 | 5.15 | 19.3 |
| 1a | 14.99 | 5.32 | 22.72 | 1100 | 0.1283 | 5.05 | 3.69 | 5.16 | 12.4 |
| 1b | 14.95 | 5.32 | 22.68 | 1100 | 0.1276 | 5.05 | 3.69 | 5.16 | 13.2 |
| 1c | 14.9 | 5.31 | 22.64 | 1100 | 0.1267 | 5.05 | 3.69 | 5.15 | 13.3 |
| 1d | 14.87 | 5.31 | 22.61 | 1100 | 0.1262 | 5.05 | 3.69 | 5.15 | 14.4 |
| 1e | 14.86 | 5.31 | 22.60 | 1100 | 0.1260 | 5.05 | 3.69 | 5.15 | 15.9 |
| 2a | 14.93 | 5.46 | 22.42 | 1200 | 0.1570 | 5.06 | 3.66 | 5.15 | 13.4 |
| 2b | 14.92 | 5.46 | 22.41 | 1200 | 0.1470 | 5.06 | 3.66 | 5.15 | 13.6 |
| 2c | 14.9 | 5.46 | 22.40 | 1200 | 0.1556 | 5.06 | 3.66 | 5.15 | 13.3 |
| 2d | 14.85 | 5.45 | 22.35 | 1200 | 0.1555 | 5.06 | 3.67 | 5.14 | 13.7 |
| 2e | 14.84 | 5.45 | 22.34 | 1200 | 0.1553 | 5.06 | 3.67 | 5.14 | 15.4 |
| 3a | 14.73 | 5.62 | 22.00 | 1300 | 0.1949 | 5.07 | 3.60 | 5.12 | 16.3 |
| 3b | 14.72 | 5.62 | 22.00 | 1300 | 0.1958 | 5.07 | 3.60 | 5.12 | 16.0 |
| 3c | 14.71 | 5.61 | 21.99 | 1300 | 0.1911 | 5.07 | 3.60 | 5.12 | 14.9 |
| 3d | 14.7 | 5.61 | 21.98 | 1300 | 0.1911 | 5.07 | 3.60 | 5.12 | 14.9 |
| 3e | 14.68 | 5.61 | 21.96 | 1300 | 0.1912 | 5.07 | 3.60 | 5.11 | 15.2 |
| 3f | 14.66 | 5.61 | 21.94 | 1300 | 0.2028 | 5.07 | 3.60 | 5.10 | 18.4 |
| 4a | 14.54 | 5.79 | 21.63 | 1400 | 0.2774 | 5.07 | 3.53 | 5.09 | 17.6 |
| 4b | 14.53 | 5.79 | 21.62 | 1400 | 0.2787 | 5.07 | 3.53 | 5.09 | 16.6 |
| 4c | 14.5 | 5.79 | 21.59 | 1400 | 0.2711 | 5.07 | 3.53 | 5.08 | 17.1 |
| 5a | 14.36 | 5.98 | 21.23 | 1500 | 0.3677 | 5.07 | 3.47 | 5.06 | 18.1 |
| 5b | 14.35 | 5.98 | 21.23 | 1500 | 0.3699 | 5.07 | 3.47 | 5.06 | 17.9 |
| 5c | 14.33 | 5.98 | 21.21 | 1500 | 0.3625 | 5.07 | 3.47 | 5.06 | 18.2 |
| 5d | 14.32 | 5.97 | 21.20 | 1500 | 0.3765 | 5.07 | 3.47 | 5.04 | 19.7 |
| 6a | 14.17 | 6.20 | 20.80 | 1600 | 0.4772 | 5.07 | 3.42 | 5.03 | 18.8 |
| 6b | 14.15 | 6.19 | 20.79 | 1600 | 0.4749 | 5.07 | 3.43 | 5.02 | 19.1 |
| 7a | 14.01 | 6.44 | 20.37 | 1700 | 0.6257 | 5.07 | 3.39 | 5.00 | 19.1 |
| 7b | 14 | 6.44 | 20.37 | 1700 | 0.6458 | 5.07 | 3.39 | 5.00 | 19.0 |
| 7c | 13.97 | 6.43 | 20.34 | 1700 | 0.6399 | 5.07 | 3.39 | 4.99 | 20.0 |
Notes. The secondary is, for every model, at the start of mass transfer in its Hertszprung gap. The final mass of the primary and secondary, Mf1 and Mf2, and the amount of hydrogen in the envelope MH are given at the time of explosion, together with the luminosity log(L/L⊙) and effective temperature Teff of the primary and secondary at the onset of central carbon burning.
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