\begin{table}%[t]%T3
%\centering
\par
     \caption{Stellar parameters of HIP~108422 and its CC are derived from the BCAH98 model for an age of 40~Myr. This model is also used for the star GSC~8047-0232, but the CBAH00 DUSTY model is used for its CC for an age of 50~Myr. }
        \label{tab:stell1}
	$$
         \begin{tabular}{llll}
            \hline  \hline       
\noalign{\smallskip}
            Source     & $M$              &  $T_{\rm{eff}}$         &$L$             \\
                       & ($M_{\odot}$)    &  (K)                 &($L_{\odot}$)  \\
        \noalign{\smallskip}
            \hline      
 \noalign{\smallskip}
           HIP~108422 & [0.9, 1.15]       & [4760,5638]      &[0.5,0.8]     \\
           HIP~108422~CC& [0.2, 0.35]      & [3301,3455]      &[0.013,0.03]     \\
        \noalign{\smallskip}
            \hline
\noalign{\smallskip}
            GSC~8047-0232 & [0.8, 0.9]      & [4203,4764]               &[0.02,0.45]     \\
        \noalign{\smallskip}
            \hline
\noalign{\smallskip}
\hline
\noalign{\smallskip}
            GSC~8047-0232~CC & [0.02, 0.04]      & [1760, 2475]      &[2e-4,8e-4]     \\
\hline
\end{tabular}
$$
\end{table}