\begin{table}%t7
\caption{Physical parameters for the two components of the \epsindibab{} 
system derived using the COND models of Baraffe \etal{} (2003) covering the 
plausible range of ages (0.8, 1.3, and 2.0~Gyr) for the system (Lachaume 
\etal{} 1999; SMLK03). See text for a detailed discussion of the derivation 
and the errors in the assumptions, as well as the masses derived in similar
fashion from the Burrows \etal{} (1997) models.
}
\label{tab:physical}
%\centering
\par
\begin{tabular}{|ccccc|ccc|ccc|ccc|}
\hline\hline
Source           & $M_K$           & $BC_K$        & $M_{\rm bol}$   &
$\log L/\Lsolar$ & 
\multicolumn{3}{c|}{Mass}          &
\multicolumn{3}{c|}{Radius}        &
\multicolumn{3}{c|}{$T_{\rm eff}$} \\
                 &                 &               &                 & 
                 &
\multicolumn{3}{c|}{\Mjup}         &
\multicolumn{3}{c|}{$R/\Rsolar$}   &
\multicolumn{3}{c|}{K}             \\
                 &                 &               &                 &
                 &
0.8              & 1.3             & 2.0           &
0.8              & 1.3             & 2.0           &
0.8              & 1.3             & 2.0           \\
\hline
\epsindiba{}     & $13\fm58$ & $2\fm88$& $16\fm46$ & 
$-4.71$          & 
38               & 47              & 57            &
0.096            & 0.091           & 0.086         &
1238             & 1276            & 1312          \\
\epsindibb{}     & $15\fm85$ & $2\fm22$& $18\fm07$ & 
$-5.35$          & 
22               & 28              & 35            &
0.101            & 0.096           & 0.092         &
835              & 854             & 875           \\
\hline
\end{tabular}
\end{table}