Supernova Remnants as Cosmic X-Ray Sources. Tycho SNR

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Supernova Remnants, Individual: Tycho, X-Rays

Scientific paper

Basic steps in history of X-ray astronomy and models of the one of the brightest cosmic X-ray sources, supernova remnants (SNRs), are described. The model of evolution of the SNR Tycho which takes into account the nonuniform ambient medium is presented for the first time. Characteristics of the SNR are found: energy of supenova explosion E = 1050 erg, ambient proton number density around the explosion position n = 1 cm-3, shock front radius Rs(theta=0) = 2.3 pc, Rs(theta=pi) = 2.1 pc, shock front velocity Ds(0) = 2200 km/s, Ds(p) = 1900 km/s, ambient proton number density in the region of the shock front n(0) = 0.75 cm-3, n(p) = 1.36 cm-3, swept-up mass M = 1.6 Msun, distance to the SNR d = 2.4 kpc.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Supernova Remnants as Cosmic X-Ray Sources. Tycho SNR 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 Supernova Remnants as Cosmic X-Ray Sources. Tycho SNR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernova Remnants as Cosmic X-Ray Sources. Tycho SNR will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-934038

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.