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Molecular Formation in Hot Diffuse Clouds

Published online by Cambridge University Press:  14 August 2015

A. Dalgarno
A. Dalgarno*
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Abstract

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A description is given of the processes of molecular formation and destruction in diffuse interstellar clouds and detailed models of the clouds lying towards ζ Ophiuchi, ζ Persei and o Persei are used to assess the validity of gas phase chemistry. Modifications that may arise from shock-heated regions are discussed.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 273 - 280
Copyright
Copyright © Reidel 1980 

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