Table B.1
Stellar and wind parameters of our model grid used to check the radiative acceleration in the B supergiant or hypergiant domain. All models have a luminosity of log L*/L⊙ = 5.76, and have been calculated with a velocity field exponent β = 1, a micro-turbulent velocity vturb = 10 km s−1, an un-clumped wind, no X-ray emission from wind-embedded shocks, and solar abundances from Asplund et al. (2009), in particular YHe=NHe/NH = 0.1.
| Model | Mass M⊙ | Teff (K) | R* (R⊙) | log g (cgs) | Γe | Ṁ (M⊙ yr−1) | υ∞ (km s−1) |
|---|---|---|---|---|---|---|---|
| B225_1 | 31.5 | 22500 | 49.3 | 2.55 | 0.43 | 8.20·10−6 | 678 |
| B225_2 | 31.5 | 22500 | 49.3 | 2.55 | 0.43 | 0.73·10−6 | 678 |
| B200_1 | 30.1 | 20000 | 62.4 | 2.33 | 0.45 | 11.20.10−6 | 556 |
| B200_2 | 50.5 | 20000 | 62.4 | 2.55 | 0.27 | 3.70·10−6 | 560 |
| B175_1 | 33.0 | 17500 | 71.3 | 2.25 | 0.31 | 14.30.10−6 | 397 |
| B175_2 | 33.0 | 17500 | 71.3 | 2.25 | 0.31 | 3.00.10−6 | 430 |
| B150_1 | 37.8 | 15000 | 83.2 | 2.17 | 0.20 | 14.30.10−6 | 397 |
| B150_2 | 45.0 | 15000 | 83.2 | 2.25 | 0.17 | 3.50.10−6 | 430 |
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