Physics
Scientific paper
Mar 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998sussp...3..490h&link_type=abstract
Shevchenko Ukrainian Scientific Society, Reports and Articles, Physics Series, Vol. 3, p. 490
Physics
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.
Hnatyk Bohdan
Petruk O.
No associations
LandOfFree
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.
Profile ID: LFWR-SCP-O-934038