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Table A.2

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)

h0a 13.5 5.10 21.52 1000 0.0835 5.03 3.86 4.96 32.2
h0b 14 5.13 21.98 1000 0.0886 5.03 3.82 5.01 31.7
h0c 14.85 5.19 22.76 1000 0.0980 5.04 3.76 5.09 30.3
h1a 13.3 5.16 21.25 1100 0.0997 5.03 3.76 4.94 32.3
h1b 13.4 5.17 21.34 1100 0.1014 5.04 3.76 4.95 32.2
h1c 14 5.23 21.85 1100 0.1111 5.04 3.73 5.00 31.7
h1d 14.85 5.31 22.59 1100 0.1258 5.05 3.69 5.08 30.2
h2a 13.2 5.31 20.86 1200 0.0983 5.05 3.78 4.92 32.2
h2b 13.3 5.32 20.95 1200 0.1012 5.04 3.77 4.93 32.1
h2c 14 5.37 21.60 1200 0.1195 5.06 3.72 4.99 31.5
h2d 14.8 5.45 22.31 1200 0.1450 5.06 3.67 5.07 30.1
h2e 14.83 5.45 22.33 1200 0.1450 5.06 3.67 5.07 30.1
h3a 12.1 5.35 19.65 1300 0.0983 5.06 3.78 4.80 32.6
h3b 12.2 5.36 19.75 1300 0.1079 5.06 3.77 4.81 32.5
h3c 14.64 5.61 21.93 1300 0.2009 5.07 3.60 5.04 30.5
h4a 11.4 CONTACT / 1400 / / / / /
h4b 11.5 5.43 18.85 1400 0.1223 5.06 3.72 4.74 32.5
h4c 11.9 5.47 19.29 1400 0.1329 5.06 3.69 4.77 32.6
h4d 12 5.48 19.38 1400 0.1430 5.07 3.68 4.78 32.6
h4e 14.49 5.79 21.58 1400 0.2785 5.07 3.53 5.01 30.8
h5a 11.1 CONTACT / 1500 / / / / /
h5b 11.2 5.56 18.37 1500 0.1615 5.07 3.65 4.70 32.4
h5c 11.6 5.60 18.84 1500 0.1843 5.07 3.62 4.73 32.5
h5d 13 5.79 20.06 1500 0.2711 5.07 3.53 4.86 32.3
h5e 14 5.93 20.92 1500 0.3538 5.07 3.48 4.95 31.4
h5f 14.31 5.97 21.19 1500 0.3604 5.07 3.47 4.98 31.0
h6a 10.7 CONTACT / 1600 / / / / /
h6b 10.8 5.68 17.81 1600 0.2183 5.07 3.58 4.64 32.4
h6c 11.3 5.76 18.36 1600 0.2442 5.07 3.55 4.69 32.5
h6d 13 6.01 19.81 1600 0.3916 5.07 3.46 4.84 32.2
h6e 14.1 6.19 20.73 1600 0.4740 5.07 3.43 4.94 31.2
h6f 14.14 6.19 20.77 1600 0.4862 5.07 3.43 4.95 31.1
h7a 10.4 CONTACT / 1700 / / / / /
h7b 10.5 5.81 17.34 1700 0.2716 5.08 3.53 4.61 32.1
h7c 11.1 5.91 17.98 1700 0.3318 5.08 3.50 4.66 32.3
h7d 11.4 5.96 18.23 1700 0.3468 5.08 3.48 4.68 32.4
h7e 12.7 6.20 19.31 1700 0.4784 5.07 3.42 4.80 32.2
h7f 12.8 6.21 19.38 1700 0.5041 5.07 3.42 4.81 32.2
h8a 10.3 CONTACT / 1800 / / / / /
h8b 10.4 5.95 17.08 1800 0.3467 5.08 3.49 4.58 32.0
h8c 11 6.05 17.70 1800 0.4006 5.08 3.45 4.63 32.4
h8d 11.5 6.16 18.11 1800 0.4668 5.08 3.43 4.68 32.2
h8e 11.8 6.22 18.34 1800 0.4860 5.08 3.42 4.70 32.2
h8f 11.9 6.24 18.41 1800 0.5104 5.08 3.42 4.71 32.2
h9a 10.3 CONTACT / 1900 / / / / /
h9b 10.4 6.12 16.95 1900 0.4531 5.08 3.44 4.57 31.8
h9c 10.8 6.19 17.24 1900 0.4873 5.08 3.42 4.60 28.8
h9d 10.9 6.22 17.31 1900 0.5014 5.08 3.42 4.61 32.0

Notes. The secondary is, for every model, at the start of mass transfer a main sequence star. The other symbols have a similar meaning as in Table A.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 “/”.

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