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Table A.5

Parameters of the atmosphere models with mass-loss rates not scaled with metallicity and at Z = 0.01 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⊙
149.5 65950 4.46 6.379 11.92 −5.00 4141 0.01 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
145.3 64470 4.40 6.387 12.59 −4.89 3898 0.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
136.9 62095 4.30 6.396 13.71 −4.71 3498 1.00 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
122.5 60486 4.20 6.402 14.55 −4.45 3051 1.50 0.702 0.298 1.545 10−6 8.703 10−5 4.203 10−7
103.6 62714 4.19 6.403 13.55 −4.38 2804 2.00 0.527 0.473 9.491 10−7 8.773 10−5 4.042 10−7
81.0 70365 4.29 6.396 10.67 −4.25 2714 2.50 0.263 0.737 1.328 10−6 8.732 10−5 3.708 10−7
200 M⊙
197.9 67602 4.44 6.564 14.03 −4.70 4122 0.01 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
187.4 65799 4.37 6.563 14.80 −4.57 3799 0.50 0.751 0.249 1.422 10−5 2.014 10−5 6.024 10−5
170.9 64269 4.29 6.563 15.51 −4.36 3402 1.00 0.715 0.285 1.709 10−6 8.685 10−5 4.078 10−7
146.4 65803 4.27 6.556 14.67 −4.30 3119 1.50 0.572 0.428 1.624 10−6 8.696 10−5 3.963 10−7
120.0 69940 4.30 6.546 12.85 −4.20 2942 2.00 0.365 0.635 1.730 10−6 8.685 10−5 3.752 10−7
83.4 82277 4.46 6.510 8.90 −4.10 2797 2.50 0.094 0.906 2.051 10−6 8.653 10−5 3.233 10−7
250 M⊙
247.4 68733 4.43 6.700 15.87 −4.49 4128 0.03 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
232.3 66802 4.36 6.693 16.68 −4.37 3788 0.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
207.6 66804 4.32 6.684 16.50 −4.25 3498 1.00 0.664 0.336 1.753 10−6 8.681 10−5 3.950 10−7
175.8 68824 4.31 6.674 15.36 −4.16 3231 1.50 0.504 0.496 1.783 10−6 8.679 10−5 3.818 10−7
137.6 73957 4.35 6.652 12.97 −4.07 3012 2.00 0.284 0.716 1.897 10−6 8.668 10−5 3.570 10−7
99.4 84863 4.49 6.610 9.38 −3.99 2874 2.40 0.072 0.928 2.128 10−6 8.645 10−5 3.094 10−7
300 M⊙
299.5 69809 4.43 6.810 17.47 −4.33 4160 0.02 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
273.6 67652 4.35 6.796 18.30 −4.22 3731 0.50 0.744 0.256 1.777 10−6 8.678 10−5 3.931 10−7
241.1 68494 4.33 6.783 17.59 −4.14 3502 1.00 0.625 0.375 1.796 10−6 8.677 10−5 3.852 10−7
197.4 70950 4.32 6.767 16.09 −4.06 3158 1.50 0.453 0.547 1.847 10−6 8.672 10−5 3.708 10−7
151.1 76698 4.37 6.736 13.29 −3.98 2960 2.00 0.226 0.774 1.969 10−6 8.661 10−5 3.429 10−7
117.8 85051 4.48 6.698 10.34 −3.92 2888 2.30 − 0.931 2.157 10−6 8.642 10−5 3.040 10−7

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 circles in Fig. 1).

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