No CrossRef data available.
Article contents
Before and After Herschel – Modeling Photo-Induced Chemistry and PDR Line Emission in the Warm and Dense ISM (WADI)
Published online by Cambridge University Press: 25 November 2011
Abstract
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.
- 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