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.
star $\log~T_{\rm {eff}}$ $\log~L_\star/L_{\odot}$ $M_\star (M_{\odot}$ ) $R_\star (R_\odot)$ $v_{\rm crit}$ $R_{\rm s} (R_\odot)$ $v_{\rm lim}$ $\Gamma_{\rm e}$ $\alpha$ k $\sigma _{\rm e}$ $\dot{M}_{\rm CAK}$ $v_\infty$

O5IV 4.60 5.7 40 18 535 19.8 525 0.326 0.640 0.124 0.34 3.72 10^-6 1257

B5II 4.30 5.0 30 30 435 33.0 430 0.016 0.565 0.320 0.31 0.65 10^-6 1074

**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.
star	$\log~T_{\rm {eff}}$	$\log~L_\star/L_{\odot}$	$M_\star (M_{\odot}$ )	$R_\star (R_\odot)$	$v_{\rm crit}$	$R_{\rm s} (R_\odot)$	$v_{\rm lim}$	$\Gamma_{\rm e}$	$\alpha$	k	$\sigma _{\rm e}$	$\dot{M}_{\rm CAK}$	$v_\infty$
O5IV	4.60	5.7	40	18	535	19.8	525	0.326	0.640	0.124	0.34	3.72 10^-6	1257
B5II	4.30	5.0	30	30	435	33.0	430	0.016	0.565	0.320	0.31	0.65 10^-6	1074

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