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Theoretical models of Herbig-Haro objects

Published online by Cambridge University Press:  04 August 2017

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

Abstract

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A brief overview of the observational characteristics of HH objects is given. Current models for their production by the interaction of stellar winds and jets with interstellar gas are critically discussed. Models for two specific systems of HH objects, namely, the Orion HH objects and the HH46-47 system are described with reference to the general production mechanisms.

Type
Herbig-Haro Objects
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 159 - 172
Copyright
Copyright © Reidel 1987 

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