Thin Layer Approximation in 3-D
天体物理学
2009-10-30 v1
摘要
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.
引用
@article{arxiv.astro-ph/9707188,
title = {Thin Layer Approximation in 3-D},
author = {G. S. Bisnovatyi-Kogan and S. A. Silich},
journal= {arXiv preprint arXiv:astro-ph/9707188},
year = {2009}
}
备注
4 pages, 2 figures