\begin{table}%t5
\caption{Stability of P-type orbits in binary systems.}\label{tab5}
%\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
    2 & 0.60 & 22.0 & 2.20 &  U\\      
      &      & 23.0 & 2.30 & MS\\
      &      & 24.0 & 2.40 &  S\\
\hline
    4 & 0.33 & 11.0 & 2.20 &  U\\      
      &      & 11.1 & 2.22 & MS\\
      &      & 11.2 & 2.24 &  S\\
\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}