Hydrodynamics of young supernova remnants

Details Hydrodynamics of young supernova remnants Hydrodynamics of young supernova remnants

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565...59b&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 59-68 (2001).

Astronomy and Astrophysics

Astrophysics

7

Supernova Remnants, Pre-Main Sequence Objects, Young Stellar Objects And Protostars, Pulsars

Scientific paper

The structure and evolution of young supernova remnants are determined, to a large extent, by using the equations of ideal, compressible gas dynamics to evolve a hypersonically expanding ejecta propagating into an ambient gas. Even within this limited domain of ideal gas dynamics, this simple problem can become extremely complex. Here we review some of the hydrodynamic solutions describing young supernova remnants, from one-dimensional self-similar models to three-dimensional simulations incorporating nonuniform ejecta. An online version of the conference presentation is available at http://wonka.physics.ncsu.edu/~blondin/october2000 .

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