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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

Bührke, T. & Mundt, R, 1987, this volume.Google Scholar
Falle, S.A.E.G. & Wilson, M.J., 1985, Mon. Not. Roy. Astr. Soc., 216, 79.Google Scholar
Glaz, H.M. & Wardlaw, A.B., 1985, J. Comput. Phys., 58, 157.Google Scholar
Mundt, R., Brugel, E.W. & Bührke, T, 1986, preprint.Google Scholar
Mundt, R. & Fried, J.W., 1983, Astrophys. J. Letters, 274, L83.Google Scholar
Prandtl, L., 1952, Fluid Dynamics, (Blackie: London).Google Scholar
Reipurth, B., Bally, J., Graham, J.A., Lane, A. & Zealey, W.J., 1986, Astron. & Astrophys., in press.Google Scholar
Sanders, R.H., 1983, Astrophys. J., 266, 73.CrossRefGoogle Scholar
Wilson, M.J. & Falle, S.A.E.G., 1985, Mon. Not. Roy. Astr. Soc., 216, 971.Google Scholar