\begin{table}%T3
      \caption{Stability of orbits in mean motion resonances. The numbers
        give the stable orbits according to the 8 different initial conditions.}
         \label{tab3} 
%\centerline
 {
\begin{tabular}{lcccccccccc}
            \hline\hline
 %           \noalign{\smallskip}
&\multicolumn{2}{c}{Gl 777 A}&\multicolumn{2}{c}{47 Uma$^a$}&\multicolumn{2}{c}{HD
            72659}&\multicolumn{2}{c}{Gl 614$^b$}&\multicolumn{2}{c}{HD 4208$^c$}\\
\hline    
%\noalign{\smallskip}
& P & A & Mode I & Mode II & P  & A  & P  & A  & P & A\\
\hline    
%\noalign{\smallskip}
5:1& 1 & 0 & 8  & 6   & 8  & 8  & 0  & 0  & 8 & 8 \\
4:1& 0 & 0 & 3  & 0   & 8  & 8  & 0  & 0  & 8 & 8 \\
3:1& 0 & 0 & 0  & 0   & 4  & 3  & 0  & 0  & 8 & 7 \\
5:2& 0 & 0 & 6  & 7   & 2  & 2  & 0  & 0  & 3 & 2 \\
7:3& 0 & 0 & 1  & 1   & 1  & 0  & 0  & 0  & 8 & 8 \\
2:1& 0 & 0 & 1  & 2   & 3  & 3  & 0  & 0  & 8 & 8 \\
5:3& 0 & 0 & -- & --  & 2  & 1  & -- & -- & 7 & 5 \\
3:2& 2 & 1 & -- & --  & 0  & 2  & 0  & 0  & 7 & 8 \\
4:3& 0 & 0 & 4  & 0   & -- & -- & -- & -- & 3 & 1 \\
\hline
%\noalign{\smallskip}
Sum [\%]& 4.7 & 1.6 & 28.6 & 69.6& 42.2 & 43.8 & 0.0 & 0.0 & 83.3 & 76.4 \\
Total Sum [\%] & \multicolumn{2}{c}{3.1} & \multicolumn{2}{c}{34.9} & \multicolumn{2}{c}{43.0} & \multicolumn{2}{c}{0.0} & \multicolumn{2}{c}{79.9}\\
            \hline
            \noalign{\smallskip}
\end{tabular}}
$^a$ Note that in
            the case of the 47 Uma system, 
            where two
            Jovian planets are known, we did not use peri- and apoastron
            position as initial conditions, but 2 different modes
            corresponding to an aligned or anti-aligned configuration of the
            two major bodies. \\
$^b$ Besides the 7 given
            resonances, we calculated the motion inside the 7:2, 9:2 and 8:3
            resonance -- again, we only found unstable
            motion. \\
$^c$ For this system, we
            calculated all resonances up to the 4th order (see
            Sect.~4); with the exceptions of the 15:11 and the 13:9 MMRs the other resonant positions showed
            the same amount of predominantly stable motion.                              
\end{table}