Table 1: Stellar parameters of the 9 non-rotating models for which the maximum mass-loss rates were determined in Paper I. The line force parameters $\alpha $ and k are taken from Pauldrach et al. (1986). The critical velocity $v_{\rm crit}$ is expressed in km s-1 while $\sigma _{\rm e}$ is expressed in cm2 g-1. The mass-loss rate is given in units of 10-6 $M_{\odot }$ yr-1.
Model $\log~L/L_{\odot}$ $T_{\mbox{eff}}$ $M (M_{\odot}$) $R (R_\odot)$ $\Gamma$ $v_{\rm crit}$ $\alpha $ k $\sigma _{\rm e}$ $\dot{M}_{\rm max}^{\rm eq}$
Model 1 6.0 50 000 K 60 15 0.434 873 0.64 0.124 0.34 4.3
Model 2 6.0 40 000 K 50 23 0.521 644 0.64 0.124 0.34 6.1
Model 3 6.0 30 000 K 40 42 0.613 426 0.59 0.17 0.32 11.8
Model 4 5.5 40 000 K 40 10 0.209 873 0.64 0.124 0.34 0.8
Model 5 5.5 30 000 K 35 18 0.221 609 0.59 0.17 0.32 1.0
Model 6 5.5 20 000 K 30 40 0.250 378 0.565 0.32 0.31 3.4
Model 7 5.0 40 000 K 30 8 0.087 846 0.64 0.124 0.34 0.1
Model 8 5.0 30 000 K 25 14 0.089 584 0.59 0.17 0.32 0.2
Model 9 5.0 20 000 K 20 32 0.119 345 0.565 0.32 0.31 0.5


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