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Table 1.

Properties of our selected evolutionary tracks at the end of the H-core burning stage.

Mzams Wind recipe vrot, ini vrot vrot, final τMS Mtotal MHe − core Ysurf N/C N/O ϵ(N) Rmax

[M] [km s−1] [Myr] [M] [M] Mass fraction By number [R]
85 sc 409.0 323.1 87.2 3.600 80.07 34.92 0.470 5.726 2.334 8.011 35.2
85 Vink 435.0 319.0 26.0 3.594 77.24 38.39 0.538 9.794 3.837 8.136 26.1
60 sc 379.0 354.7 111.0 4.192 57.33 20.42 0.378 3.482 1.294 7.837 29.1
60 Vink 400.0 317.0 85.0 4.197 56.34 21.77 0.402 4.740 1.648 7.901 27.5
40 sc 348.0 323.1 210.0 5.398 39.06 8.43 0.327 3.163 0.950 7.745 21.7
40 Vink 358.0 300.0 125.0 5.253 38.67 9.81 0.314 3.218 0.916 7.725 21.4
32 sc 331.0 299.1 258.0 6.624 31.52 4.83 0.336 4.478 1.053 7.791 17.5
32 Vink 338.0 282.0 177.0 6.354 31.24 5.74 0.310 4.072 0.927 7.739 16.4
25 sc 314.0 272.9 285.0 8.551 24.79 1.16 0.356 7.380 1.205 7.849 13.9
25 Vink 319.0 262.0 132.0 7.663 24.67 2.04 0.292 4.655 0.862 7.721 13.8
20 sc 300.0 252.0 277.0 10.513 19.93 0.12 0.336 8.849 1.143 7.833 11.5
20 Vink 305.0 248.0 194.0 9.238 19.87 0.11 0.277 4.736 0.792 7.697 11.6

Notes. Values for tracks adopting Vink’s formula are taken from Georgy et al. (2013), with ϵ(N) = log(N/H)+12.

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