Thermal X-ray emission of the remnants of ashperical Supernova explosions
Abstract
Description
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.
4 pages, 1 figure; contribution to a Conference "Astronomy in Ukraine - 2000 and beyond (Impact of International Cooperation)" (5-8.06.2000, Kyiv, Ukraine)
4 pages, 1 figure; contribution to a Conference "Astronomy in Ukraine - 2000 and beyond (Impact of International Cooperation)" (5-8.06.2000, Kyiv, Ukraine)