\begin{table}%t5
\caption{Masses of the components derived from orbital solution I.}\label{tab5}
%\centering
\par
\begin{tabular}{ccc}
\hline  \hline
$M_1 \sin^3{i}$ & $M_2 \sin^3{i}$ & $q=M_2/M_1$\\
 $1.84 \pm 0.02~M_{\sun}$&
 $0.654\pm 0.006~M_{\sun}$&
 $0.355\pm 0.001$\\
\hline
\end{tabular}
\end{table}