Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae 2013/12/18 Speaker : Yu-Hsun Cheng Professor: Yosuke Mizuno.
Facts about SNe and their remnants
Shock modification at the rim of SN 1006
Wei W. Liu, Tong-Jiang Wang, Brian R. Dennis, Gordon D. Holman submitted to ApJ on 11 Feb 2009
Facts about SNe and their remnants Evolution of an SNR sensitively depends on its environment. Observed SNRs are typically produced by SNe in relative.
Image: Toward high-resolved hydrodynamic Simulations of Supernova remnants such as Cas A, Tycho.. Masaomi Ono.
Starburst episodes in low luminosity AGN
