Online Material

$\begin{figure} \par\includegraphics[width=16cm,clip]{figure1_near1.eps} \end{figure}$	Figure 1: Observed SED and their best fit models. Filled circular symbols represent the data points and the filled triangles represent photometry used as upper limits on the fitting. The dashed line corresponds to the stellar photosphere model used in the best YSO model fit.
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$\begin{figure} \par\includegraphics[width=16cm,clip]{figure1_near2.eps} \end{figure}$	Figure 1: continued.
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$\begin{figure} \par\includegraphics[width=16cm,clip]{figure1_near3.eps} \end{figure}$	Figure 1: continued.
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$\begin{figure} \par\includegraphics[width=16cm,clip]{figure1_far1.eps} \end{figure}$	Figure 1: continued.
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$\begin{figure} \par\includegraphics[width=16cm,clip]{figure1_far2.eps} \end{figure}$	Figure 1: continued.
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$\begin{figure} \par\includegraphics[width=16cm,clip]{figure1_far3.eps} \end{figure}$	Figure 1: continued.
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Table 1: Parameters obtained for all the sources in our sample.