\begin{table}%T3
%\renewcommand{\arraystretch}{1.3}
\caption{The physical parameters of the two young eclipsing binaries \object{RX~J0529.4+0041~A} and \object{V1174~Ori} as adopted from \citet{Covino04} and \citet{Stassun04}, respectively. We use their temperature solutions but also determine a set of additional effective temperatures using other temperature scales (see Sect.~\ref{sect:temp}).
\label{tab:EclBin}}
%\centering
\par
\begin{tabular}{l|ll}
\hline
\hline
&\object{RX~J0529.4+0041 Aa}&\object{RX~J0529.4+0041 Ab}\\
\hline
$M~[M_{\odot}]$&$1.27\pm0.01$&$0.93\pm0.01$\\
$R~[R_{\odot}]$&$1.44\pm0.05$&$1.35\pm0.05$\\
${\log}~g~[{\rm cgs}]$&$4.22\pm0.02$&$4.14\pm0.02$\\
$T_{\rm eff}~$[K]&$5200\pm150$&$4220\pm150$\\
spectral type&K1$\pm$1&K7-M0\\
\hline
&\object{V~1174~Ori~A}&\object{V~1174~Ori~B}\\
\hline
$M~[M_{\odot}]$&$1.009\pm0.015$&$0.731\pm0.008$\\
$R~[R_{\odot}]$&$1.339\pm0.015$&$1.065\pm0.011$\\
${\log}~g~[{\rm cgs}]$&$4.19\pm0.01$&$4.25\pm0.01$\\
$T_{\rm eff}~$&$4470\pm120$&$3615\pm100$\\
spectral type&K4.5~$\pm$~0.5&M~1.5\\
\hline
\end{tabular}   
\end{table}