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Interstellar Wind-Blown Bubbles

Published online by Cambridge University Press:  12 April 2016

J. E. Dyson
J. E. Dyson*
Affiliation:
Department of Astronomy, University of Manchester, England

Summary

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‘Classical’ stellar wind-driven bubbles are either energy or momentum driven, and evolve in smooth media containing only radial density gradients. Real bubbles are produced from winds from moving stars and which blow into non-homogeneous media. The resulting mixing of clump material can produce a variety of thermal, dynamical and chemical effects. In this review we discuss some of the modifications to classical bubbles which ensue, using observational examples where appropriate.

Type
II. Mechanical Energy Sources
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 136 - 145
Copyright
Copyright © Springer-Verlag 1989

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