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Table A.6

Parameters of the atmosphere models with mass-loss rates scaled linearly with Z 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⊙
150.5 66051 4.46 6.385 11.96 −6.59 4138 0.01 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
149.9 64726 4.40 6.408 12.79 −6.48 3903 0.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
150.2 62531 4.31 6.409 14.20 −6.31 3593 1.00 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
150.5 58739 4.17 6.471 16.70 −6.14 3194 1.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
148.7 51769 3.91 6.506 22.39 −5.95 2586 2.00 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
149.7 37868 3.33 6.546 43.71 −5.73 1738 2.50 0.249 2.491 10−5 7.295 10−6 6.040 10−5
200 M⊙
201.9 67673 4.45 6.564 14.01 −6.31 4206 0.01 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
200.7 66125 4.38 6.592 15.14 −6.17 3894 0.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
199.4 63209 4.27 6.620 17.13 −6.01 3494 1.00 0.751 0.249 2.471 10−5 7.698 10−6 6.035 10−5
197.9 57802 4.08 6.652 21.24 −5.84 2954 1.50 0.751 0.249 2.471 10−5 7.698 10−6 6.035 10−5
197.0 47388 3.70 6.685 32.82 −5.66 2210 2.00 0.751 0.249 2.471 10−5 7.698 10−6 6.035 10−5
198.3 35520 3.18 6.707 59.91 −5.53 2756 2.30 0.751 0.249 2.467 10−5 7.750 10−6 6.035 10−5
250 M⊙
251.6 68911 4.44 6.701 15.82 −6.10 4200 0.02 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
251.9 67088 4.37 6.725 17.16 −5.97 3904 0.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
247.6 63509 4.24 6.753 19.76 −5.83 3403 1.00 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
249.0 56482 4.01 6.781 25.80 −5.67 2832 1.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
249.3 41849 3.46 6.811 48.67 −5.50 1924 2.00 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
300 M⊙
298.1 69895 4.43 6.810 17.42 −5.94 4141 0.02 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
297.1 67656 4.35 6.832 19.07 −5.83 3796 0.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
301.7 63487 4.22 6.858 22.32 −5.69 3403 1.00 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
296.9 55111 3.94 6.885 30.56 −5.54 2663 1.50 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5
294.1 36252 3.18 6.914 73.01 −5.37 1555 2.00 0.751 0.249 2.491 10−5 7.295 10−6 6.040 10−5

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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