Thin Layer Approximation in 3-D

Details Thin Layer Approximation in 3-D Thin Layer Approximation in 3-D

1997-07-16

arxiv.org/abs/astro-ph/9707188v1

Proc. IAU Coll. 166

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures

Scientific paper

10.1007/BFb0104708

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

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