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Table 2

Stellar and wind parameters of our grid models with homogeneous winds, following Pauldrach et al. (2001).

Model Teff log g R* v
(kK) (cm s−2) (R) (km s−1) (10−6 yr−1)
Dwarfs
D30 30 3.85 12 1800 0.008
D35 35 3.80 11 2100 0.05
D40 40 3.75 10 2400 0.24
D45 45 3.90 12 3000 1.3
D50 50 4.00 12 3200 5.6
D55 55 4.10 15 3300 20

Supergiants
S30 30 3.00 27 1500 5.0
S35 35 3.30 21 1900 8.0
S40 40 3.60 19 2200 10
S45 45 3.80 20 2500 15
S50 50 3.90 20 3200 24

Notes. Forall models, the velocity field exponent has been set to β = 0.9, and a micro-turbulent velocity, vturb = 15 km s−1, has been used.

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