X-ray emission of the remnants of aspherical supernova explosions

Details X-ray emission of the remnants of aspherical supernova explosions X-ray emission of the remnants of aspherical supernova explosions

Sep 2000

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

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 132-135

Physics

Scientific paper

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

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