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Before and After Herschel – Modeling Photo-Induced Chemistryand PDR Line Emission in the Warm and Dense ISM (WADI)

Published online by Cambridge University Press:  25 November 2011

M. Röllig ,
R. Simon ,
V. Ossenkopf ,
J. Stutzki ,
M. Röllig ,
C. Dedes ,
Ch. Joblin  and
V. Ossenkopf
M. Röllig
Affiliation:
I. Physikalisches Institut der Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany. e-mail: roellig@ph1.uni-koeln.de ,
C. Dedes
Affiliation:
Institute for Astronomy, ETH Zürich, 8093 Zürich, Switzerland
Ch. Joblin
Affiliation:
Université de Toulouse, UPS, CESR, 31062 Toulouse Cedex 4, France
V. Ossenkopf
Affiliation:
SRON Netherlands Institute for Space Research, 9700 AV Groningen, The Netherlands
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Abstract

We present HIFI observations of [CII] and high-J transitions of CO and HCO+ atpositions in S140 and DR21. We use a clumpy PDR model to model and interpret the observedline intensities. The emission from both massive star forming regions can be reproduced byassuming a clumpy, 2-component PDR scenario.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 52: Conditions and Impact of Star Formation , 2011 , pp. 301 - 302
Copyright
© EAS, EDP Sciences 2011

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References

Dedes, C., et al., 2010, A&A, 521, L24
Ossenkopf, V., et al., 2010, A&A, 518, L79
Röllig, M., et al., 2006, A&A, 451, 917