Gamma-radiation from the accretion of supernova envelope on compact remnant
The numerical simulation of massive envelope of a star during supernova type II explosion with the compact object was done. The characteristic time when the envelope becomes transparent and the supernova remnant can be observed in gamma rays was estimated. The parameters of the supernova were chosen to correspond to observable characteristics of SN 1987A.
supernovae, SN 1987A
Publication language:russian, pages:15
Mathematical modelling in actual problems of science and technics