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Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium

Tomasz Plewa·Michal Rozyczka
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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.

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Tomasz Plewa, Michal Rozyczka. 1996-07-06. Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium. https://arxiv.org/abs/astro-ph/9607039

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