\begin{table}%[ht]%T2
\caption{Lifetimes of Wolf-Rayet star from various initial masses and velocities
and predictions for different number ratios (see text). The velocities are in~km~s$^{-1}$ and the lifetimes in Myr.} 
\label{tblwr}
%\centerline
{%\scriptsize
\begin{tabular}{ccccccc}\hline\hline
$M$   & $v_{\rm ini}$        & $t_{\rm WR}$ & $t_{e\rm WNL}$ & $t_{e\rm WNE}$ & $t_{\rm WN/WC}$ & $t_{\rm WC}$  \\
    &                   &          &           &           &             &           \\[-2.2mm]
\hline
    &                   &          &           &           &             &           \\[-2.2mm]
120 & 0                 & 0.6767   & 0.3499    & 0.0265    & 0.0038      & 0.2965    \\ 
    & 300               & 1.3969   & 1.0402    & 0.0706    & 0.0010      & 0.2851    \\
    &                   &          &           &           &             &           \\
 85 & 0                 & 0.4846   & 0.1941    & 0.0231    & 0.0000      & 0.2674    \\ 
    & 300               & 1.4050   & 1.0707    & 0.1263    & 0.0065      & 0.2015    \\
    &                   &          &           &           &             &           \\
 60 & 0                 & 0.3732   & 0.0838    & 0.0808    & 0.0000      & 0.2086    \\
    & 300               & 0.7527   & 0.4489    & 0.0562    & 0.0202      & 0.2274    \\
    & 300I              & 0.7779   & 0.4734    & 0.0346    & 0.0343      &    0.2356 \\
    & 500               & 1.0787   & 0.7250    & 0.0816    & 0.0206      &    0.2515 \\
    & 500I              & 1.0703   & 0.7312    & 0.0628    & 0.0211      &   0.2552  \\
    &                   &          &           &           &             &           \\
 40 & 0                 & 0.0714   & 0.0317    & 0.0397    & 0.0000      & 0.0000    \\
    & 300               & 0.3670   & 0.1478    & 0.0000    & 0.0447      & 0.1745    \\
    &                   &          &           &           &             &           \\
 25$^1$ & 0                 & 0.0000   & 0.0000    & 0.0000    & 0.0000      & 0.0000    \\
    & 300               & 0.2068   & 0.2068    & 0.0000    & 0.0000      & 0.0000    \\[-1.2mm]
    &                   &          &           &           &             &           \\[-2.2mm]
\hline
    &                   &          &           &           &             &           \\[-2.2mm]
 \multispan{7}\hfill Predicted number ratios \hfill \\[-2.2mm]
    &                   &          &           &           &             &           \\
 $v_{\rm ini}$        & ${\rm WR} \over {\rm O}$       & ${\rm eWNL}\over {\rm WR}$   
 & ${\rm eWNE}\over {\rm WR}$   & ${\rm WN/WC}\over {\rm WR}$  & ${\rm WC}\over {\rm WR}$  & ${{\rm WC}\over {\rm WN}}^{2}$     \\[-1.2mm]
                      &          &           &           &             &        &           \\[-1.2mm]
\hline
                      &          &           &           &             &        &           \\[-3.2mm]
    0                 & 0.02     & 0.35      & 0.16      & 0.00        & 0.49   &  0.97     \\[-1.2mm] 
                      &          &           &           &             &        &           \\[-1.2mm]
    300               & 0.07     & 0.66      & 0.05      & 0.04        & 0.25   &  0.35     \\[-1.2mm]
                      &          &           &           &             &        &           \\[-1.2mm]
\hline   
\end{tabular}}
\par
\medskip                     
$^1$ $M_{\min}$ for WR star formation from a single star is 37 and 22 for \mbox{$\upsilon_{\rm ini}=0$}, 300~km~s$^{-1}$ respectively.\\[0.5mm]
$^2$ WC/WN = WC/(WNL+WNE). 
\end{table}