Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium
| dc.creator | Plewa, Tomasz | |
| dc.creator | Rozyczka, Michal | |
| dc.date | 1996-07-06 | |
| dc.date.accessioned | 2026-07-07T02:21:27Z | |
| dc.date.available | 2026-07-07T02:21:27Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9607039 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9607039 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10554 | |
| dc.subject | Astrophysics | |
| dc.title | Modern Numerical Hydrodynamics and the Evolution of Dense Interstellar Medium | |
| dc.type | text |