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JD14 – Examining the PDR-molecular cloud interface at mm and IR wavelengths

Published online by Cambridge University Press:  21 October 2010

R. Simon ,
V. Ossenkopf  and
M. Röllig
R. Simon
Affiliation:
I. Physikalisches Institut, Universität zu Köln, Germany email: simonr@ph1.uni-koeln.de, ossk@ph1.uni-koeln.de, roellig@ph1.uni-koeln.de, stutzki@ph1.uni-koeln.de
V. Ossenkopf
Affiliation:
I. Physikalisches Institut, Universität zu Köln, Germany email: simonr@ph1.uni-koeln.de, ossk@ph1.uni-koeln.de, roellig@ph1.uni-koeln.de, stutzki@ph1.uni-koeln.de
M. Röllig
Affiliation:
I. Physikalisches Institut, Universität zu Köln, Germany email: simonr@ph1.uni-koeln.de, ossk@ph1.uni-koeln.de, roellig@ph1.uni-koeln.de, stutzki@ph1.uni-koeln.de
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Abstract

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Much progress has been made in recent years towards a better understanding of the physical and chemical processes in Photo-dissociation/Photon-dominated Regions (PDRs), both observationally and in terms of detailed physical and chemical modelling. This article highlights some of the problems and new opportunities observers and modellers are facing.

Keywords

astrochemistryISM: cloudsISM: evolutionISM: kinematics and dynamicsISM: structureradio lines: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 399 - 400
Copyright
Copyright © International Astronomical Union 2010

References

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