\begin{table}%t3
\caption{\label{tab:models}Best-fit solutions of the two methods the system of 809~Lundia based on the fit of photometric observations made in 2005$-$2006  and 2006$-$2007 (see Fig.~\ref{f9}).}
%\centering
\small                                 
\begin{tabular}{c c c c c c c c c c c c c}
\hline 
\hline
Model    &\multicolumn{3}{c}{Component A} & \multicolumn{3}{c}{Component B}& Separation & Mass      & Density    & Period          & \multicolumn{2}{c}{Pole of orbit} \\
         &\multicolumn{3}{c}{ km }        & \multicolumn{3}{c}{ km}        &   km       & ratio     & $\rm g/cm^3$   &  h              & $\lambda$~deg & $\beta$~deg \\
         & $a$   &$b$    &$c$                   &    $a'$  & $b'$  & $c'$              &            &           &            &                 &               &    \\
\hline
Modified & 3.9 & 3.3 & 3.2                &    3.5 & 2.9 & 2.8             &  15.8      &0.7 $\pm$ 0.1& 1.64 $\pm$ 0.1&15.418 $\pm$ 0.001& 119 $\pm$ 2     & 28 $\pm$ 4 \\
Roche    &     &     &                    &        &     &                 &            &           &            &                 &               &          \\     
Kinematic& 4.1 & 3.3 & 2.5                &    3.2 & 2.9 & 2.7             &  15.8      &0.7 $\pm$ 0.1& 1.71 $\pm$ 0.1&15.418 $\pm$ 0.001& 120 $\pm$ 5     & 18 $\pm$ 12 \\  
         &     &     &                    &        &     &                 &            &           &            &                 &               &           \\
\hline
\end{tabular}       
\end{table}