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

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

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....52..301r&link_type=abstract

EAS Publications Series, Volume 52, 2011, pp.301-302

Computer Science

Scientific paper

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

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