\begin{table}%t9
\caption{\label{tab9}Assumed parameters used in computing the models.}
%\centerline
 {\begin{tabular}{lll}
\hline\hline
Parameter & Adopted value & Explanation \\
\hline \\[-8pt]
$\dot{M}_{{\rm WR}}$ & $1.6\times 10^{-5}$ $M_{\odot}$~yr$^{-1}$ & 
mass-loss rate$^{{a}}$ \\
$v_{\infty,{\rm WR}}$ & 1785 km~s$^{-1}$ & terminal 
velocity$^{{b,c}}$ \\
$T_{\ast}$ & 32~000 K & WR temperature$^{{d}}$ \\
$v_{0,{\rm WR}}$ & 60 km~s$^{-1}$ & initial velocity \\
$R_{\ast}^{{\rm WR}}$ & 11.9~$R_{\odot}$ & stellar radius$^{{a}}$ \\
$\dot{M}_{{\rm O}}$ & $2.8\times 10^{-7}$~$M_{\odot}$~yr$^{-1}$ & 
mass-loss rate$^{{e}}$ \\
$v_{\infty,{\rm O}}$ & 2100 km~s$^{-1}$ & terminal velocity$^{{e}}$ \\
$R_{\ast}^{{\rm O}}$ & 8 to 13~$R_{\odot}$ & stellar radius \\
\\
$i$ & 70\degr or 85\degr & System inclination$^{{a}}$ \\
& & (two test values) \\
\hline
\end{tabular}}
\par
\smallskip
$^{{a}}$ Rauw (\cite{rauw97});
$^{{b}}$ Hamann et~al.\ (\cite{hama06});
$^{{c}}$ Crowther et~al.\ (\cite{crow95b});\\
$^{{d}}$ Lamers \& Morris (\cite{lamo94});
$^{{e}}$ Vink et~al.\ (\cite{vink01}).
\end{table}