EDP Sciences
Free Access
Issue
A&A
Volume 498, Number 1, April IV 2009
Page(s) 147 - 159
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/200810902
Published online 24 February 2009

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.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=16cm,clip]{figure1_near2.eps}
\end{figure} Figure 1:

continued.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=16cm,clip]{figure1_near3.eps}
\end{figure} Figure 1:

continued.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=16cm,clip]{figure1_far1.eps}
\end{figure} Figure 1:

continued.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=16cm,clip]{figure1_far2.eps}
\end{figure} Figure 1:

continued.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=16cm,clip]{figure1_far3.eps}
\end{figure} Figure 1:

continued.

Open with DEXTER

Table 1:   Parameters obtained for all the sources in our sample.


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