\begin{table}%t3
%\centering
\par
 \caption{Estimated accretion rates from the CaII($\lambda8542$)
line.}\label{t3}
\begin{tabular}{lcc} \noalign{\smallskip}\hline\hline
\noalign{\smallskip}
Object & ${\cal F}_{\rm CaII(\lambda 8542)}{\rm (erg \ s^{-1})}$ &
${\dot M} {  (M_\odot \ {\rm yr}^{-1})}$ \\
\noalign{\smallskip}\hline \noalign{\smallskip}
\object{Sz100} & $5.2 \times 10^{29}$ & $1.9 \times 10^{-8}$\\
\object{Sz102} & $2.0 \times 10^{29}$ & $7.9 \times 10^{-9}$\\
\object{Sz106}$^1$ & $2.0 \times 10^{28}$ & $1.0 \times 10^{-9}$\\
\object{Sz113} & $1.8 \times 10^{29}$ & $7.2 \times 10^{-9}$\\
\noalign{\medskip}
\object{Par-Lup3-4} & $2.8 \times 10^{28}$ & $1.4 \times 10^{-9}$\\
\object{LS-RCrA~1} & $4.7 \times 10^{27}$ & $2.8 \times 10^{-10}$\\
\noalign{\smallskip}\hline\noalign{\smallskip}
\multicolumn{3}{l}{$^1$ $I_{\rm C}$ estimated from the FORS1 images.}\\
\end{tabular}
\end{table}