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A jet model of Herbig-Haro objects

Published online by Cambridge University Press:  04 August 2017

M. J. Wilson ,
S.A.E.G. Falle  and
D. E. Innes
M. J. Wilson
Affiliation:
Department of Applied Mathematics, The University Leeds LS2 9JT
S.A.E.G. Falle
Affiliation:
Max-Planck-Institüt für Kernphysik, Postfach 10 39 80, D-6900 Heidelberg
D. E. Innes
Affiliation:
Max-Planck-Institüt für Kernphysik, Postfach 10 39 80, D-6900 Heidelberg

Abstract

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We present results of steady jet calculations in which the cooling and compression behind internal shocks leads to optical emission with an intensity pattern similar to the regular well-aligned emission knots characteristic of stellar jets.

Type
Herbig-Haro Objects
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 193 - 194
Copyright
Copyright © Reidel 1987 

References

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