\begin{table}%T3
\par
\caption{\label{models}Models results for candidate ZAMS sources in the field.}
\small%\centerline
{
\begin{tabular}{lcccccccccc}\hline\hline
Sou. & $M_{\star}$ & $T_{\star}$ & $R_{\star}$ & $R_{\rm Disk}$ & $i$ & $A_{\rm V}$ & $L_{\rm bol}^a$ & Log[$N_{\rm Ly}$] & $G_0$ \\
 & [$M_{\odot}$] & [K] & [$R_{\odot}$] & [AU] & [\adeg] & [mag] & \lsun &  [s$^{-1}$] &  \\
  \hline
B  & 11.4 & 27~500 & 4.3 & 380 & 87 & 15.5 & 9400 & 46.3 & 200 \\
C  & 9.7 &  25~300 & 3.9 & 2000 & 70 & 11.5 & 5600 & 45.8 & 120 \\
D & 10.0 & 25~600 & 4.0 & 660 & 87 & 7.3 & 6400 & 45.9 & 135 \\
H & 6.0 & 18~400 & 2.9 & 410 & 87 & 0.0 & 900 & 43.4 & 10 \\
I  & 9.2 & 24~500 & 3.8 & 120 & 70 & 6.2 & 4700 & 45.8 & 50 \\ 
\hline
\end{tabular}}
\smallskip
 $^a$ As given by the models. 
\end{table}