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

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

2001-03-26

arxiv.org/abs/astro-ph/0103412v1

Kinematics and Physics of Celestial Bodies, Suppl. Ser., 2000, No 3

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure; contribution to a Conference "Astronomy in Ukraine - 2000 and beyond (Impact of International Cooperation)"

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.

Affiliated with

Also associated with

No associations

Rating

Thermal X-ray emission of the remnants of ashperical Supernova explosions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Thermal X-ray emission of the remnants of ashperical Supernova explosions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Thermal X-ray emission of the remnants of ashperical Supernova explosions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-33158