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Table 1
Input stellar and wind parameters of our models.
| Model | L⋆ | M⋆ | R⋆ | log g | Teff | α |  |
Qmax | vesc,eff | ṀVink |
|---|---|---|---|---|---|---|---|---|---|---|
| [L⊙] | [M⊙] | [R⊙] | [g cm−3] | [kK] | [ ] |
[km s−1] | [M⊙ yr−1] | |||
| OSG1 | 6 × 105 | 40 | 20 | 3.43 | 35 | 0.6 | 2000 | 0.004 | 678 | 4.1 × 10−6 |
| OSG2 | 4 × 105 | 30 | 20 | 3.31 | 30 | 0.6 | 2000 | 0.004 | 608 | 1.5 × 10−6 |
| BSG1 | 1 × 105 | 20 | 40 | 2.53 | 20 | 0.5 | 2000 | 0.004 | 407 | 7.0 × 10−7 |
| BSG2 | 6 × 104 | 20 | 40 | 2.53 | 15 | 0.5 | 2000 | 0.004 | 419 | 3.2 × 10−7 |
Notes. For comparison we include mass-loss rates as predicted by Vink et al. (2001) using the ratios v∞ ∕vesc, eff = 1.3, 2.6 for below and above the bi-stability, respectively.
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