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Table 1

Properties of source-star models.

Model M ini V ini / V crit Ωini/ Ωcrit V eq,ini Initial τ life τ MS τ He τ C τ Ne τ O τ Si M MS M He M final
[M] [km s-1] composition [Myr] [Myr] [Myr] [yr] [day] [day] [day] [M] [M] [M]

No rotation

20s0 20 0 0 0 α-enhanced 8.93 8.02 0.79 978 168 318 3.1 19.99 19.98 19.98
32s0 32 0 0 0 α-enhanced 5.78 5.24 0.48 124 22 47 0.6 31.97 31.94 31.94
60s0 60 0 0 0 α-enhanced 3.81 3.44 0.33 15 7 7 0.5 59.87 59.81 59.80

Rotation

20s7 20 0.7 0.88 610 α-enhanced 11.0 10.1 0.76 400 277 128 1.4 19.84 19.84 19.50
32s7 32 0.7 0.88 680 α-enhanced 7.14 6.61 0.47 45 7 15 0.6 31.48 31.42 30.71
60s7 60 0.7 0.88 770 α-enhanced 4.69 4.33 0.32 5 1 3 0.2 58.47 47.97 47.65

Notes. The table includes: model name (Col. 1) initial mass (Col. 2), Vini/Vcrit (Col. 3), Ωini/ Ωcrit (Col. 4), initial equatorial velocity (Col. 5), initial composition (Col. 6), total lifetime (Col. 7), lifetime of the MS, helium, carbon, neon, oxygen, and silicon-burning phases (Cols. 7–13), mass of the model at the end of MS, helium-burning phase, and at the end of evolution (Cols. 14–16).

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