\begin{table}%t1
\caption{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. (\cite{Pau86}).  The
classical CAK mass loss and CAK terminal wind velocity are also listed.
$\sigma_{\rm e}$ is expressed in cm$^2$ g$^{-1}$, $\dot{M}_{\rm CAK}$ in
$M_\odot~$yr$^{-1}$ and $v_\infty$ in km~s$^{-1}$. }
%\centering
\par
\begin{tabular}{cccccccccccccc}
\hline  \hline
star & $\log~T_{\rm {eff}}$ & $\log~L_\star/L_{\odot}$ & $M_\star 
(M_{\odot}$) & 
$R_\star (R_\odot)$ & $v_{\rm crit}$ & $R_{\rm s} (R_\odot)$ & $v_{\rm lim}$ & 
$\Gamma_{\rm e}$ & $\alpha$ & $k$ & $\sigma_{\rm e}$ & $\dot{M}_{\rm CAK}$ &
$v_\infty$ \\
\hline
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\\
\hline
\end{tabular}
\label{par}
\end{table}