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Basic Problems of Planetary Nebula Gas Dynamics

Published online by Cambridge University Press:  07 August 2017

J.E. Dyson
J.E. Dyson*
Affiliation:
Department of Astronomy, University of Manchester, Manchester M13 9PL, U.K.

Abstract

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Planetary Nebulae result from the interaction of fast winds and radiation fields with slow ejecta produced in the late stages of evolution of moderately low mass stars. We review the basic principles of the interaction and describe some of the modifications needed to produce realistic models for comparison with observational data. The present status of numerical modelling is discussed and some important problems outlined.

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 299 - 306
Copyright
Copyright © Kluwer 1993 

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