X-ray emission of the remnants of ashperical Supernova explosions

Details X-ray emission of the remnants of ashperical Supernova explosions X-ray emission of the remnants of ashperical Supernova explosions

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kpcbs...3..132p&link_type=abstract

Kinematics and Physics of Celestial Bodies, Supplement, vol. 3, p. 132

Physics

Suprnova Remnants, X-Rays, Hydrodynamics, Aspherical Explosion

Scientific paper

Evolution of adiabatic remnants of an aspherical supernova explosion in uniform medium are considered. Thermal X-ray emission of such remnants are investigated. It is shown that integral thermal X-ray characteristics (X-ray luminosity and spectrum) of the objects do not allow us to reveal the assymetry in the explosion because these characteristics are close to their Sedov counterparts. Surface distribution of X-ray emission is sensitive to anisotropy of the explosion and nonuniformity of the interstellar medium.

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