Thermal X-ray emission of the remnants of ashperical Supernova explosions
| dc.creator | Petruk, O. | |
| dc.date | 2001-03-26 | |
| dc.date.accessioned | 2026-07-07T01:58:01Z | |
| dc.date.available | 2026-07-07T01:58:01Z | |
| dc.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. | |
| dc.description | 4 pages, 1 figure; contribution to a Conference "Astronomy in Ukraine - 2000 and beyond (Impact of International Cooperation)" (5-8.06.2000, Kyiv, Ukraine) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0103412 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0103412 | |
| dc.identifier | Kinematics and Physics of Celestial Bodies, Suppl. Ser., 2000, No 3 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2613 | |
| dc.subject | Astrophysics | |
| dc.title | Thermal X-ray emission of the remnants of ashperical Supernova explosions | |
| dc.type | text |