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Supernova explosions in stellar wind bubbles

Published online by Cambridge University Press:  19 July 2016

S. Jane Arthur
S. Jane Arthur*
Affiliation:
Department of Applied Mathematics, The University, Leeds LS2 9JT, UK

Abstract

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Type II supernovae play a major role in the dynamics of the interstellar medium. The interstellar medium in which such supernovae evolve is often considerably modified by the strong stellar winds both from the progenitor and other nearby stars. The result is that the appearance and energetics of the remnants can be very different from that of remnants in a uniform medium. In this paper we will consider the evolution of supernova remnants in stellar wind bubbles including the effect of departures from spherical symmetry. The aim is to understand both the appearance of such remnants and their effect on the overall energetics of the interstellar medium.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 331 - 333
Copyright
Copyright © Kluwer 1991 

References

Arthur, S.J.: 1990, Multigrid Methods Applied to a Point Explosion at a Plane Density Interface , in preparation.Google Scholar
Brandt, A.: 1977, Multi-level adaptive techniques (MLAT) for partial differential equations: Ideas and Software in Mathematical Software III (Rice, J.R. ed.), Academic Press, New York.Google Scholar
Meaburn, J.: 1978, Astrophys. Space Sci. , 59, 193.CrossRefGoogle Scholar
Sedov, L.I.: 1959, Similarity and Dimensional Methods in Mechanics , Academic Press, New York.Google Scholar
Steger, J.L. and Warming, R.F.: 1981, J. Comp. Phys. , 40, 263.Google Scholar