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Table A.4

Parameters of the atmosphere models with mass-loss rates scaled linearly with Z and at Z = 0.1 Z⊙.

M M⊙ Teff K log g log(L/L⊙) R R⊙ log⁡ M˙$\[\log~ \dot{M}\]$ v∞ km s−1 age Myr H He C N O
150 M⊙
150 61566 4.34 6.378 13.66 −5.63 3862 0.01 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
148.6 59236 4.25 6.402 15.16 −5.49 3591 0.50 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
146.7 56821 4.14 6.427 16.97 −5.33 3219 1.00 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
143.8 52448 3.97 6.454 20.54 −5.15 2804 1.50 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
139.2 43724 3.61 6.483 30.56 −4.92 2119 2.00 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
130.4 22079 2.36 6.518 124.76 −4.59 896 2.50 0.745 0.253 7.566 10−5 5.361 10−4 2.600 10−4
200 M⊙
200 63321 4.33 6.564 15.99 −5.32 3897 0.00 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
197.2 60169 4.22 6.584 18.13 −5.18 3565 0.51 0.748 0.251 2.167 10−4 9.790 10−5 5.757 10−4
193.2 56682 4.08 6.607 20.97 −5.02 3107 1.01 0.748 0.251 1.269 10−4 2.027 10−4 5.752 10−4
187.2 49803 3.82 6.631 27.93 −4.82 2509 1.50 0.748 0.251 3.687 10−5 3.069 10−4 5.743 10−4
176.9 35628 3.18 6.660 56.41 −4.56 1502 2.00 0.731 0.268 1.393 10−5 8.305 10−4 5.919 10−6
170.7 26821 2.66 6.673 101.06 −4.46 1067 2.20 0.691 0.307 1.399 10−5 8.314 10−4 4.795 10−6
250 M⊙
249.8 63530 4.30 6.699 18.57 −5.11 3884 0.03 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
245.6 60640 4.19 6.717 20.80 −4.98 3474 0.50 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
239.3 56146 4.03 6.738 24.86 −4.82 3024 1.00 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
229.6 46858 3.67 6.761 36.65 −4.60 2206 1.50 0.748 0.251 2.068 10−4 1.546 10−4 5.214 10−4
213.7 30564 2.87 6.789 88.95 −4.40 1231 2.00 0.670 0.328 1.432 10−5 8.311 10−4 4.665 10−6
300 M⊙
300 64263 4.29 6.807 20.54 −4.96 3868 0.00 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
293.9 60705 4.17 6.823 23.45 −4.84 3477 0.50 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
285.1 55047 3.96 6.842 29.16 −4.67 2813 1.00 0.748 0.251 2.379 10−4 6.967 10−5 5.769 10−4
271.5 44384 3.55 6.865 46.02 −4.47 2046 1.50 0.724 0.275 1.443 10−5 8.309 10−4 4.760 10−6
250.3 23967 2.41 6.892 162.86 −4.28 893 2.00 0.624 0.375 1.460 10−5 8.309 10−4 4.541 10−6

Notes. Columns are mass of the corresponding model according to stellar evolution rounded up to the first decimal, effective temperature, surface gravity, luminosity, radius, mass-loss rate, wind terminal velocity, age, and surface abundances of H,He, C,N, and O given in mass fraction. For each mass, the lines of this table correspond to the characteristics of the models marked as filled squares in Fig. 1).

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