\begin{table}%t1
\caption{\label{fit}Parameters obtained using the SED fitting tool of Robitaille et~al.~(\cite{rob07}) for the brightest PACS 
100~$\mu$m sources. }
\small%\centering
\par
\begin{tabular}{l r c c c}
\hline\hline\noalign{\smallskip}
  YSO & $M_{\rm star}$  & 
   $\dot{M}_{\rm envelope}$ & $M_{\rm envelope}$ & $L$ \\
     & ($M_{\odot}$)  & (10$^{-4}$~$M_{\odot}$~yr$^{-1}$) & ($M_{\odot}$)&  ($L_{\odot}$) \\
  \hline
\multicolumn{5}{l}{Condensation~1}\\
%\hline
\#0  &  8--10 & 80 & 1000    & 2~$\times$~10$^{3}$ \\
\#36 & 1.0  & 5 & 8 & 15  \\
\#38 & 3--4  & 10 & 50--100 & 150  \\
\hline
\multicolumn{5}{l}{Condensation~2}\\
%\hline
\#50 & 2--3 & 1 & 8 & 300 \\
\hline
\multicolumn{5}{l}{Condensation~4}\\
%\hline
\#69 & 1.5  & 8 & 100 & 70  \\
\#76 & 0.8 & 3 & 10 & 10 \\
\hline
\multicolumn{5}{l}{Condensation~5}\\
%\hline
\#105 & 1.0  & 80 & 100 & 20 \\
\hline
\multicolumn{5}{l}{Condensation~6}\\
%\hline
\#106 & 1.5  & 8 & 100 & 50 \\
\hline
  \end{tabular}
\vspace{-3mm}
\end{table}