\begin{table}%t3
\caption{Dependence of orbital stability on mass of secondary star.}\label{tab3}
%\centerline
{
\begin{tabular}{c c c c c}
\hline
\hline
Binary & $M_{\rm B}/M_{\rm A}$ & $R_{\rm AG}$ & $R_{\rm AG}/R_{\rm AB}$ 
& Orbital\\
system & \omit & [AU] & \omit & stability\\
\hline
    3 & 0.20 & 2.56 & 0.32 &  S\\      
      & 0.40 & 2.56 & 0.32 & MS\\
      & 0.60 & 2.56 & 0.32 & MS\\
      & 0.80 & 2.56 & 0.32 &  U\\
\hline
\end{tabular}}
\medskip
Note: Simulations were performed for giant planets with $M_{\rm G}$~= 1~$M_{\rm Jup}$ based on 1000~orbits.
\end{table}