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A model of the distribution of ionised carbon in M17SW

Published online by Cambridge University Press:  03 August 2017

Simon Pinnock  and
Tania S. Monteiro
Simon Pinnock
Affiliation:
Queen Mary & Westfield College, Mile End Road, London, E1 4NS.
Tania S. Monteiro
Affiliation:
Queen Mary & Westfield College, Mile End Road, London, E1 4NS.

Abstract

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The observed distribution of ionised carbon with depth into the edge-on photodissociation region (PDR) in M17SW is not consistent with results from chemical models which assume a constant or smoothly varying density. These observations have been interpreted to indicate that the PDR actually consists of many clumps embedded in a low density interclump medium (1). A chemical model is described which is designed to simulate such a clumpy PDR.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 485 - 486
Copyright
Copyright © Kluwer 1991 

References

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