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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 Vink
[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 vvesc, eff = 1.3, 2.6 for below and above the bi-stability, respectively.

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