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Thin Layer Approximation in 3-D

Published online by Cambridge University Press:  12 April 2016

G.S. Bisnovatyi-Kogan  and
S.A. Silich
G.S. Bisnovatyi-Kogan
Affiliation:
Space Research Institute, 84/32 Profsoyuznaya, Moscow, 117810, Russia
S.A. Silich
Affiliation:
Main Astronomical Observatory of the National Academy of Sciences of Ukraine 252650, Kiev, Golosiiv, Ukraine

Abstract

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Equations are derived which describe the propagation of strong shocks in the interstellar matter, without any restrictions for symmetry, in a thin layer approximation (2.5 dimensions). Using these equations permits to calculate the propagation of shock waves from nonsymmetric supernovae explosions in a medium with arbitrary density distribution and the formation of superbubbles in galaxies.

Type
Part III Observations and Modeling of the Local Bubble and the SXRB
Information
International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 137 - 140
Copyright
Copyright © Springer-Verlag 1998

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