Observational study of sites of triggered star formation - CO and mid-infrared observations

J. S. Urquhart; L. K. Morgan; M. A. Thompson

doi:10.1051/0004-6361/200811149

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Volume 497 / No 3 (April III 2009)

A&A, 497 3 (2009) 789-804

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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

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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.

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