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Table 6

Stellar properties at the end of hot phase, when Teff decreases below 15 000 K for the first time.

Hot wind algorithm MZAMS [ M ] η R [ R ] L [ 104L ] M [ M ] MHe [ M ] Age [Myr]

V 15 1.0 34.85 5.44 14.54 3.69 12.7917
K 15 1.0 35.44 5.64 14.73 3.71 12.8239

V 15 0.33 35.91 5.76 14.85 3.76 12.7503
K 15 0.33 35.97 5.82 14.91 3.77 12.7612

V 15 0.1 36.27 5.85 14.95 3.78 12.7363
K 15 0.1 35.96 5.83 14.97 3.78 12.7359

V 20 1.0 51.97 12.20 19.06 5.83 8.8937
K 20 1.0 52.75 12.32 19.42 5.87 8.8947

V 20 0.33 53.10 12.67 19.69 5.95 8.8373
K 20 0.33 53.35 12.76 19.81 5.95 8.8374

V 20 0.1 53.46 12.80 19.91 5.99 8.8176
K 20 0.1 54.39 13.10 19.94 5.98 8.8183

V 25 1.0 67.58 20.63 23.24 8.03 7.0367
K 25 1.0 68.70 21.41 24.00 7.91 7.0094

V 25 0.33 70.59 22.55 24.44 7.97 6.9653
K 25 0.33 70.05 22.04 24.66 8.07 6.9546

V 25 0.1 70.88 22.39 24.84 8.10 6.9390
K 25 0.1 70.50 22.19 24.90 8.13 6.9355

V 30 1.0 80.82 29.52 27.00 10.18 5.9700
K 30 1.0 84.32 31.82 28.46 10.00 5.9215

V 30 0.33 84.64 32.11 29.10 10.16 5.8853
K 30 0.33 85.14 32.83 29.48 10.11 5.8689

V 30 0.1 85.58 32.85 29.77 9.96 5.8558
K 30 0.1 85.34 32.93 29.84 9.89 5.8503

V 35 1.0 95.27 40.28 30.32 12.29 5.2807
K 35 1.0 97.93 41.83 32.83 12.51 5.2164

V 35 0.33 98.15 43.52 33.62 12.19 5.1879
K 35 0.33 99.84 44.24 34.27 12.09 5.1661

V 35 0.1 100.81 45.59 34.63 11.58 5.1559
K 35 0.1 100.35 45.03 34.78 11.78 5.1484

Notes. For the descriptions of the V and K algorithms see Sects. A.1 and A.2, respectively.

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