Hydrodynamic instabilities in young supernova remnants

Details Hydrodynamic instabilities in young supernova remnants Hydrodynamic instabilities in young supernova remnants

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..dppfz2002c&link_type=abstract

American Physical Society, 47th Annual DPP Meeting, October 24-28, 2005, abstract #FZ2.002

Physics

Scientific paper

The expansion of a supernova shock wave is subject to a variety of
hydrodynamic instabilities as it moves through a massive star and into
the surrounding medium. The same is true for the expansion of a
relativistic wind nebula created by a central pulsar. In many cases, the
results of the instabilities can be directly observed.

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