\begin{table}%t4
%\centering
\par
\caption{\label{mala}Comparison of resulting WR masses and orbital periods from 
non-rotating and rotating binary systems with the same initial parameters.$M_{\rm 1,in},M_{\rm 2,in}$ are
initial primary and secondary mass, $p_{\rm in}$ is the initial orbital period,
$M_{\rm WR,5}$, $M_{\rm WR,1}$ are WR masses at $X_{\rm s}=0.05$ and $X_{\rm s}\le0.01$ respectively
and $p$ is the orbital period in the initial WR+O system where the hydrogen surface abundance of WR star is 
$X_{\rm s}=0.05$. Systems are modelled with WR stellar wind mass loss H/6 except $^{\rm *}$ 
which are done with H/3, $^{\rm R}$ indicates rotating models.}
\begin{tabular}{@{\extracolsep{\fill}}lcccc}
\hline
\hline
$M_{\rm 1,in}+M_{\rm 2,in}$ & $p_{\rm in}$ & $M_{\rm WR,5}$ & $M_{\rm WR,1}$ & $p$\\
$[{M}_{\odot}]$ &  $[\rm d]$ & $[{M}_{\odot}]$ & $[{M}_{\odot}]$ & $\rm [d]$ \\   
\hline
$41+20$ &    $6$ &  $11.8$  &    $11.2$  & $12.6$\\     
$41+20^{\rm R}$ &  $6$ &  $11.0$  &    $10.2$ & $9.8$\\     
$41+24$ &    $6$ &  $12.1$  &    $11.4$  & $21.5$\\     
$41+24^{\rm R}$ &  $6$ &  $11.2$  &    $10.5$ & $16.4$\\     
$56+33^{\rm *}$ &    $6$ &  $18.6$  &    $17.5$ & $13.8$\\ 
$56+33^{\rm *,R}$ &  $6$ &  $14.9$  &    $13.6$ & $8.5$\\    
\hline
\end{tabular}
\end{table}