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Diagnosing the ISM in star-forming regions

Published online by Cambridge University Press:  21 October 2010

Willem A. Baan ,
Edo Loenen  and
Marco Spaans
Willem A. Baan
Affiliation:
ASTRON, Dwingeloo, The Netherlands
Edo Loenen
Affiliation:
ASTRON, Dwingeloo, The Netherlands Kapteyn Institute, Groningen, The Netherlands
Marco Spaans
Affiliation:
Kapteyn Institute, Groningen, The Netherlands
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Abstract

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A report on studies using the observed line ratios of high-density molecular tracers to diagnose the physics and chemistry of the ISM in star-formation environments.

Keywords

Stars: formationISM: moleculesRadio lines: ISMGalaxies: starburst
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 411
Copyright
Copyright © International Astronomical Union 2010

References

Baan, W. A., Henkel, C, Loenen, A. F, Baudry, A., & Wiklind, T 2008, A&A 477, 747Google Scholar
Baan, W. A., Loenen, A. F., & Spaans, M. 2009, A&A submittedGoogle Scholar
Loenen, A. F., Spaans, M., Baan, W. A., & Meijerink, R. 2008, A&A 488, L5.Google Scholar
Loenen, A. F., Baan, W. A., & Spaans, M 2009, A&A submittedGoogle Scholar