\begin{table}%t2
\caption{Stability of S-type orbits in binary systems.}\label{tab2}
%\centerline
{
\begin{tabular}{c c c c}
\hline
\hline
Binary & $R_{\rm AG}$ & $R_{\rm AG}/R_{\rm AB}$ & Orbital\\ 
system & [AU] & \omit & stability\\
\hline
    1 & 3.000 & 0.200 &  S\\      
      & 4.000 & 0.275 & MS\\
      & 4.750 & 0.320 & MS\\
      & 4.850 & 0.325 &  U\\
\hline
    2 & 2.000 & 0.200 &  S\\      
      & 2.750 & 0.275 & MS\\
      & 3.200 & 0.320 & MS\\
      & 3.250 & 0.325 &  U\\
\hline
    3 & 1.600 & 0.200 &  S\\      
      & 2.200 & 0.275 & MS\\
      & 2.560 & 0.320 & MS\\
      & 2.600 & 0.325 &  U\\
\hline
    4 & 1.000 & 0.200 &  S\\      
      & 1.375 & 0.275 &  S\\
      & 1.600 & 0.320 & MS\\
      & 1.625 & 0.325 & MS\\
      & 2.000 & 0.400 &  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}