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Table A.1

Parameters of the atmosphere models with mass-loss rates not scaled with metallicity and at Z = 0.2 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⊙
149.9 60415 4.31 6.379 14.20 −5.01 3815 0.01 0.746 0.252 3.921 10−4 1.148 10−4 9.508 10−4
144.6 57642 4.20 6.386 15.73 −4.90 3447 0.50 0.746 0.252 3.921 10−4 1.148 10−4 9.508 10−4
137 54852 4.09 6.396 17.57 −4.73 3132 1.00 0.746 0.251 3.921 10−4 1.148 10−4 9.508 10−4
125 51673 3.93 6.404 19.98 −4.53 2626 1.50 0.709 0.289 2.156 10−5 1.371 10−3 9.002 10−6
122.7 51490 3.85 6.407 20.19 −4.35 2316 2.00 0.534 0.464 2.171 10−5 1.371 10−3 8.290 10−6
82.5 54443 3.84 6.401 17.93 −4.25 2081 2.50 0.263 0.735 2.359 10−5 1.370 10−3 7.592 10−6
200 M⊙
201.0 61745 4.29 6.565 16.84 −4.69 3837 0.00 0.746 0.252 3.921 10−4 1.148 10−4 9.508 10−4
188.1 58232 4.16 6.563 18.88 −4.59 3384 0.50 0.746 0.252 3.895 10−4 1.200 10−4 9.504 10−4
173.8 55451 4.04 6.563 20.87 −4.42 2985 1.00 0.716 0.282 2.215 10−5 1.370 10−3 9.574 10−6
151.9 54421 3.95 6.562 21.69 −4.30 2646 1.50 0.585 0.413 2.256 10−5 1.370 10−3 8.137 10−6
123.0 54862 3.88 6.555 21.23 −4.19 1948 2.00 0.371 0.627 2.358 10−5 1.370 10−3 7.692 10−6
86.4 57821 3.85 6.523 18.37 −4.09 2003 2.50 0.091 0.906 2.658 10−5 1.367 10−3 6.638 10−6
250 M⊙
250 61207 4.23 6.698 19.98 −4.51 3693 0.00 0.746 0.252 3.921 10−4 1.148 10−4 9.508 10−4
232.5 58286 4.12 6.693 21.89 −4.38 3284 0.49 0.746 0.252 3.921 10−4 1.148 10−4 9.508 10−4
208 56272 4.02 6.688 23.37 −4.26 2929 1.00 0.669 0.329 2.273 10−5 1.370 10−3 8.088 10−6
176.9 55599 3.94 6.680 23.71 −4.16 2622 1.50 0.506 0.492 2.333 10−5 1.370 10−3 7.820 10−6
138.6 55194 3.84 6.661 23.54 −4.07 2253 2.00 0.281 0.717 2.462 10−5 1.369 10−3 7.311 10−6
111.9 54955 3.76 6.636 23.07 −4.02 1968 2.30 0.121 0.877 2.635 10−5 1.367 10−3 6.708 10−6
300 M⊙
299.9 62395 4.24 6.807 21.78 −4.35 3306 0.01 0.746 0.252 3.921 10−4 1.148 10−4 9.508 10−4
274.7 58129 4.09 6.796 24.79 −4.23 3249 0.50 0.738 0.260 2.155 10−5 1.282 10−3 1.109 10−4
241.4 56384 3.99 6.787 26.08 −4.14 2867 1.00 0.629 0.369 2.318 10−5 1.370 10−3 7.887 10−6
200.6 55562 3.90 6.774 26.46 −4.06 2528 1.50 0.451 0.547 2.390 10−5 1.369 10−3 7.586 10−6
152 53836 3.75 6.746 27.28 −3.98 2062 2.00 0.220 0.778 2.541 10−5 1.368 10−3 7.018 10−6
104.5 70779 4.10 6.707 15.09 −3.75 2049 2.40 0.000 0.998 3.365 10−5 1.361 10−3 4.386 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 open squares in Fig. 1).

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