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Table 1
Adopted parameters of the model grid (stellar effective temperature Teff, radius R∗, mass M, and luminosity L), mass-loss rates ṀVink derived using Vink et al. (2001) formula for Asplund et al. (2009) mass fraction of heavier elements, and our predicted terminal velocity v∞ and mass-loss rate Ṁ.
Model | T eff | R ∗ | M | log (L/L⊙) | Ṁ Vink | v ∞ | Ṁ | |
[ K ] | [ R⊙ ] | [ M⊙ ] | [ M⊙ yr-1] | [km s-1] | [ M⊙ yr-1] | |||
|
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Main | 300-5 | 30 000 | 6.6 | 12.9 | 4.50 | 1.3 × 10-8 | 2440 | 1.0 × 10-8 |
sequence | 325-5 | 32 500 | 7.4 | 16.4 | 4.74 | 4.2 × 10-8 | 1900 | 1.4 × 10-8 |
350-5 | 35 000 | 8.3 | 20.9 | 4.97 | 1.2 × 10-7 | 1220 | 3.8 × 10-8 | |
375-5 | 37 500 | 9.4 | 26.8 | 5.19 | 3.0 × 10-7 | 1770 | 1.1 × 10-7 | |
400-5 | 40 000 | 10.7 | 34.6 | 5.42 | 7.3 × 10-7 | 1960 | 2.5 × 10-7 | |
425-5 | 42 500 | 12.2 | 45.0 | 5.64 | 1.6 × 10-6 | 1910 | 4.5 × 10-7 | |
|
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Giants | 300-3 | 30 000 | 13.1 | 19.3 | 5.10 | 1.6 × 10-7 | 2070 | 6.2 × 10-8 |
325-3 | 32 500 | 13.4 | 22.8 | 5.25 | 3.7 × 10-7 | 1470 | 1.2 × 10-7 | |
350-3 | 35 000 | 13.9 | 27.2 | 5.41 | 8.0 × 10-7 | 1200 | 2.4 × 10-7 | |
375-3 | 37 500 | 14.4 | 32.5 | 5.57 | 1.5 × 10-6 | 1620 | 4.2 × 10-7 | |
400-3 | 40 000 | 15.0 | 39.2 | 5.71 | 2.7 × 10-6 | 1320 | 9.3 × 10-7 | |
425-3 | 42 500 | 15.6 | 47.4 | 5.85 | 4.5 × 10-6 | 1200 | 1.5 × 10-6 | |
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Supergiants | 300-1 | 30 000 | 22.4 | 28.8 | 5.56 | 9.9 × 10-7 | 1110 | 4.5 × 10-7 |
325-1 | 32 500 | 21.4 | 34.0 | 5.66 | 1.7 × 10-6 | 1140 | 5.7 × 10-7 | |
350-1 | 35 000 | 20.5 | 40.4 | 5.75 | 2.6 × 10-6 | 1350 | 6.9 × 10-7 | |
375-1 | 37 500 | 19.8 | 48.3 | 5.84 | 3.7 × 10-6 | 1260 | 1.2 × 10-6 | |
400-1 | 40 000 | 19.1 | 58.1 | 5.92 | 4.7 × 10-6 | 1460 | 1.4 × 10-6 | |
425-1 | 42 500 | 18.5 | 70.3 | 6.00 | 5.6 × 10-6 | 1350 | 1.8 × 10-6 |
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