Work

Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium

Year: 1996

Type: preprint

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.

Source: arXiv (Cornell University)

DOI: 10.48550/arxiv.astro-ph/9607039

Authors: Plewa, Tomasz, Rozyczka, Michal

Institutions: Max Planck Society, Max Planck Institute for Astrophysics, Nicolaus Copernicus Astronomical Center, University of Warsaw

Language: English

Topic: Astrophysics and Star Formation Studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

OpenAlex ID: W1808657459

Cites: 1

Cited by:

Related to: 20