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Line Emission Processes in Atomic and Molecular Shocks

Published online by Cambridge University Press:  12 April 2016

J. Michael Shull
J. Michael Shull*
Affiliation:
Center for Astrophysics and Astronomy Space, and Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards

Abstract

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This review discusses the observations and theoretical models of interstellar shock waves in diffuse and molecular clouds. After summarizing the relevant gas dynamics, atomic, molecular and grain processes, and physics of radiative and magnetic precursors, I describe observational diagnostics of shocks. I conclude with a discussion of two new topics: unstable or non-steady shocks and thermal conduction in metal-rich shocks.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 161 - 178
Copyright
Copyright © Cambridge University Press 1988

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