All Tables

Table 1: Stellar parameters of the O5IV and an B5II star for which we determined the maximum mass-loss rates as a function of equatorial rotation velocity. $\alpha$ and k are taken from Pauldrach et al. (1986). The classical CAK mass loss and CAK terminal wind velocity are also listed. $\sigma _{\rm e}$ is expressed in cm² g^-1, $\dot{M}_{\rm CAK}$ in $M_\odot~$ yr^-1 and $v_\infty$ in km s^-1.
Table 2: Maximum mass-loss rates (expressed in $10^{-6}~M_\odot$ yr^-1) for the stars with stellar parameters listed in Table 1 as a function of equatorial rotation velocity $v_{\rm eq}$ for $R_{\rm s}=1.1~R_\star$ . All $v_{\rm max}$ -values are very similar. The listed velocities are all expressed in km s^-1.
Table 3: Stellar parameters of the nine models for which we determined the maximum mass-loss rates. $\alpha$ and k are taken from Pauldrach et al. (1986). The sonic radius equals 1.01 times the stellar radius. The critical velocity at the sonic point, $v_{\rm lim}$ , is expressed in km s^-1 while $\sigma _{\rm e}$ is expressed in cm² g^-1. The last two columns give the ratio of the maximum mass-loss rates for non-rotating stars that we obtain with our formalism and the values derived from respectively classical CAK theory and the mass-loss recipe provided by Vink et al. (2000).
Table 4: Maximum mass-loss rates (expressed in $10^{-6}~M_\odot$ yr^-1) for the stellar models listed in Table 3 for $R_{\rm s}=1.01~R_\star$ . All $v_{\rm max}$ -values are very similar. The listed velocities are all expressed in km s^-1.