EDP Sciences
Free Access
Issue
A&A
Volume 497, Number 3, April III 2009
Page(s) 789 - 804
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/200811149
Published online 05 March 2009

Online Material

 \begin{figure}\par\includegraphics[width=18cm]{11149fig9-1.eps}
\par\end{figure} Figure 9:

DSS images and CO spectra obtained towards the 42 BRCs towards which emission is detected. The DSS images presented in the left panels are overlaid with contours of the MSX 8 $\mu $m emission which traces the PDR. The position of the IRAS point source associated with each cloud is indicated by a cross. Embedded MSX 21 $\mu $m point source associated with each cloud are indicated by a triangle. In the right panels we present histogram plots of the three CO transitions and the fits to the data; these are coloured in black and red respectively.

Open with DEXTER

\begin{figure}\includegraphics[width=18cm]{11149fig9-2.eps}
\par\end{figure} Figure 9:

continued.

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\begin{figure}\includegraphics[width=18cm]{11149fig9-3.eps}
\par\end{figure} Figure 9:

continued.

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\begin{figure}\includegraphics[width=18cm]{11149fig9-4.eps}
\par\end{figure} Figure 9:

continued.

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\begin{figure}\includegraphics[width=18cm]{11149fig9-5.eps}
\par\end{figure} Figure 9:

continued.

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\begin{figure}\includegraphics[width=18cm]{11149fig9-6.eps}
\par\end{figure} Figure 9:

continued.

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