Table A.4
Properties of binary stellar models for an initial primary mass of 15 M⊙, with variation of the initial secondary mass M2i, variation of the accretion efficiency β and initial orbital period Porb.
| No. | M2i | M1f | M2f | Porb | β | MH1 | log |
T eff, 1 | log |
Teff, 2 | ∗ 1/ ∗ 2 | ≠ Time |
| (M⊙) | (M⊙) | (M⊙) | (Days) | (M⊙) | (103 K) | (103 K) | (yr) | |||||
|
|
||||||||||||
| 8.5 | 14.9 | 5.15 | 18.86 | 800 | 0.50 | 0.0897 | 5.04 | 3.84 | 5.08 | 3.56 | *1 | / |
| 9.9 | 14.9 | 5.13 | 22.07 | 900 | 0.90 | 0.0814 | 5.03 | 3.84 | 5.14 | 12.6 | *1 | / |
| 9.5 | 14.9 | 5.38 | 18.75 | 900 | 0.50 | 0.1671 | 5.04 | 3.71 | 5.10 | 3.55 | *2 | 11 900 |
| 0c9 | 14.9 | 5.23 | 21.97 | 1000 | 0.90 | 0.1050 | 5.04 | 3.73 | 5.13 | 11.8 | *1 | / |
| 1b9 | 14.95 | 5.50 | 21.41 | 1100 | 0.90 | 0.2107 | 5.05 | 3.66 | 5.08 | 3.62 | *2 | 20 200 |
| 1b7 | 14.95 | 5.60 | 19.93 | 1100 | 0.70 | 0.2469 | 5.05 | 3.62 | 5.07 | 3.59 | *2 | 16 700 |
| 1c9 | 14.9 | 5.36 | 21.81 | 1100 | 0.90 | 0.1512 | 5.05 | 3.66 | 5.12 | 10.7 | *1 | / |
| 1c5 | 14.9 | 5.73 | 18.54 | 1100 | 0.50 | 0.2878 | 5.06 | 3.58 | 5.09 | 3.55 | *2 | 12 300 |
| 1d75 | 14.87 | 5.43 | 20.56 | 1100 | 0.75 | 0.1712 | 5.05 | 3.63 | 5.08 | 8.81 | *1 | / |
| 1d5 | 14.87 | 5.57 | 18.57 | 1100 | 0.50 | 0.2680 | 5.06 | 3.58 | 4.94 | 3.69 | *1 | / |
| 1d25 | 14.87 | 5.74 | 16.67 | 1100 | 0.25 | 0.2857 | 5.06 | 3.53 | 4.93 | 3.64 | *1 | / |
| 2c5 | 14.9 | 5.76 | 18.47 | 1200 | 0.50 | 0.2661 | 5.07 | 3.54 | 4.95 | 3.66 | *1 | / |
| 3d5 | 14.7 | 5.96 | 18.16 | 1300 | 0.50 | 0.3658 | 5.07 | 3.48 | 4.89 | 3.71 | *1 | / |
| 4a7 | 14.54 | 6.01 | 19.34 | 1400 | 0.70 | 0.3906 | 5.07 | 3.46 | 4.85 | 3.77 | *1 | / |
| 4c9 | 14.5 | 5.96 | 19.68 | 1400 | 0.90 | 0.3671 | 5.07 | 3.47 | 5.02 | 12.7 | *1 | / |
| 4c7 | 14.5 | 6.00 | 19.31 | 1400 | 0.70 | 0.3873 | 5.07 | 3.46 | 5.00 | 9.64 | *1 | / |
| 4c5 | 14.5 | 6.18 | 17.84 | 1400 | 0.50 | 0.4844 | 5.07 | 3.43 | 4.86 | 3.74 | *1 | / |
| g4b7 | 14.9 | 6.06 | 19.66 | 1400 | 0.70 | 0.4204 | 5.07 | 3.45 | 4.95 | 3.69 | *1 | / |
| g4c7 | 14.94 | 6.07 | 19.70 | 1400 | 0.70 | 0.4191 | 5.07 | 3.45 | 5.04 | 3.61 | *1 | / |
| g4d7 | 14.95 | 6.28 | 19.60 | 1400 | 0.70 | 0.5387 | 5.07 | 3.45 | 5.07 | 3.58 | *2 | 9700 |
| h5.0 | 8.3 | 5.37 | 10.15 | 1500 | 0.25 | 0.0795 | 5.07 | 3.87 | 3.88 | 25.1 | *1 | / |
| h5.1 | 8.6 | 5.41 | 10.44 | 1500 | 0.25 | 0.0912 | 5.07 | 3.79 | 3.93 | 25.4 | *1 | / |
| h5.2 | 8.8 | 5.44 | 10.64 | 1500 | 0.25 | 0.1074 | 5.07 | 3.75 | 3.96 | 25.5 | *1 | / |
| h5.3 | 8.8 | 5.41 | 12.49 | 1500 | 0.50 | 0.0961 | 5.07 | 3.80 | 4.17 | 27.8 | *1 | / |
| h5.4 | 9.1 | 5.44 | 12.78 | 1500 | 0.50 | 0.1164 | 5.07 | 3.75 | 4.20 | 28.0 | *1 | / |
| h5.5 | 9.4 | 5.55 | 11.22 | 1500 | 0.25 | 0.1510 | 5.07 | 3.65 | 4.06 | 26.0 | *1 | / |
| h5.6 | 9.4 | 5.49 | 13.07 | 1500 | 0.50 | 0.1239 | 5.07 | 3.70 | 4.24 | 28.2 | *1 | / |
| h5.7 | 9.4 | CONTACT | / | 1500 | 0.75 | / | / | / | / | / | / | / |
| h5.8 | 9.7 | CONTACT | / | 1500 | 0.75 | / | / | / | / | / | / | / |
| h5.9 | 10 | 5.50 | 15.49 | 1500 | 0.75 | 0.1308 | 5.07 | 3.69 | 4.46 | 30.5 | *1 | / |
| h5d5 | 14 | 6.38 | 17.23 | 1500 | 0.50 | 0.5975 | 5.07 | 3.40 | 4.43 | 27.1 | *1 | / |
| 5b9 | 14.35 | 6.06 | 20.46 | 1500 | 0.90 | 0.4163 | 5.07 | 3.45 | 5.04 | 16.6 | *1 | / |
| 5b8 | 14.35 | 6.14 | 19.72 | 1500 | 0.80 | 0.4624 | 5.07 | 3.43 | 5.01 | 14.3 | *1 | / |
| 5b75 | 14.35 | 6.19 | 19.35 | 1500 | 0.75 | 0.4886 | 5.07 | 3.43 | 4.97 | 8.67 | *1 | / |
| 5b7 | 14.35 | 6.24 | 18.97 | 1500 | 0.70 | 0.5176 | 5.07 | 3.42 | 4.84 | 3.77 | *1 | / |
| 5b6 | 14.35 | 6.34 | 18.25 | 1500 | 0.60 | 0.5750 | 5.07 | 3.40 | 4.81 | 3.78 | *1 | / |
| 5b5 | 14.35 | 6.45 | 17.54 | 1500 | 0.50 | 0.6325 | 5.07 | 3.39 | 4.81 | 3.77 | *1 | / |
| 5b25 | 14.35 | 6.74 | 15.87 | 1500 | 0.25 | 0.8062 | 5.07 | 3.37 | 4.80 | 3.72 | *1 | / |
| g5c5 | 14.55 | 6.49 | 17.72 | 1500 | 0.50 | 0.6595 | 5.07 | 3.39 | 4.85 | 3.79 | *1 | / |
| 6b9 | 14.15 | 6.29 | 20.04 | 1600 | 0.90 | 0.5445 | 5.07 | 3.41 | 5.00 | 17.5 | *1 | / |
Notes. 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. If the evolution of the binary system ended because of formation of a contact binary, the parameters cannot be determined and are indicated by “/”. The other symbols have a similar meaning as in Table A.1.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.