Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium
Astrophysics
2007-05-23 v1
Abstract
We discuss some typical problems related to numerical hydrodynamics of a dense interstellar medium. A newly developed hydrodynamical code based on adaptive mesh refinement technique is presented and applied to simulate the evolution of a supernova remnant in a high-density medium. Advantages of this new approach in comparison to commonly used hydrodynamical methods are briefly discussed.
Cite
@article{arxiv.astro-ph/9607039,
title = {Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium},
author = {Tomasz Plewa and Michal Rozyczka},
journal= {arXiv preprint arXiv:astro-ph/9607039},
year = {2007}
}
Comments
3 pages, latex, uses rmaaconf.sty, 1 Postscript figure, mpeg movies available at http://www.mpa-garching.mpg.de/Hydro/AMR/movies/starbur.html. To appear in Rev. Mex. Astr. Astrofis. (1996), proceedings of the conference "Starburst Activity in Galaxies", ed. J. Franco, R. Terlevich, and G. Tenorio-Tagle