Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium

Details Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium

1996-07-06

arxiv.org/abs/astro-ph/9607039v1

Astronomy and Astrophysics

Astrophysics

3 pages, latex, uses rmaaconf.sty, 1 Postscript figure, mpeg movies available at http://www.mpa-garching.mpg.de/Hydro/AMR/movi

Scientific paper

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.

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