Analytical Study of Supernova Remnant Non-Stationary Expansions

Details Analytical Study of Supernova Remnant Non-Stationary Expansions Analytical Study of Supernova Remnant Non-Stationary Expansions

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.298...75r&link_type=abstract

Astrophysics and Space Science, Volume 298, Issue 1-2, pp. 75-80

Astronomy and Astrophysics

Astrophysics

3

Hydrodynamics, Instabilities, Supernova Remnant, Pulsar: General

Scientific paper

We study analytically the Rayleigh Taylor instability in expanding supernova gas shell. The instability appears at the inner shell surface accelerated by blowing pulsar wind. The most dangerous perturbations correspond to wavelengths comparable to the shell thickness. We analyze the fragility of the supernova remnant shell in function of the initial perturbation amplitude and the shell thickness.

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