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Table 3.

Properties of the stellar models at the end of the main sequence.

Mzams Z vrot, ini Mass loss End of main sequence
tMS M* R* vrot, surf Ysurf N/C N/O
120.0 0.014 398.0 Vink 2.361 87.121 16.3 20.6 0.686 79.03 65.04
sc 2.603 110.15 34.6 149.0 0.687 55.86 26.31
120.0 0.006 419.0 Vink 2.513 100.504 16.5 79.7 0.694 71.32 57.79
sc 3.070 111.196 43.4 131.0 0.694 28.94 11.14

70.0 0.014 360.0 Vink 4.199 42.679 18.7 7.1 0.894 73.30 69.46
sc 3.935 60.363 26.9 3.9 0.628 18.20 5.64
70.0 0.006 376.0 Vink 3.882 57.250 15.5 37.0 0.694 34.00 13.38
sc 3.956 64.60 21.7 26.2 0.509 8.04 2.44

40.0 0.014 321.0 Vink 5.794 31.86 19.2 9.9 0.553 13.86 3.90
sc 5.535 36.428 23.6 37.4 0.460 5.46 1.50
40.0 0.006 334.0 Vink 5.622 36.196 16.2 30.6 0.440 6.101 1.647
sc 5.382 38.180 18.5 71.7 0.370 3.664 0.953

25.0 0.014 291.0 Vink 7.977 23.591 15.9 68.4 0.343 3.316 0.756
sc 7.623 24.274 16.0 113.0 0.320 2.618 0.587
25.0 0.006 302.0 Vink 7.708 24.272 14.1 159.0 0.309 3.389 0.687
sc 8.105 24.567 16.7 185.0 0.331 4.267 0.786

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