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Thin Layer Approximation in 3-D
Published online by Cambridge University Press: 12 April 2016
Abstract
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