(1) Space Research Institute of the USSR Academy of Sciences, Moscow, U.S.S.R.;(2) Sternberg State Astronomical Institute, Moscow, U.S.S.R.;(3) Main Astronomical Observatory of the Ukrainian Academy of Sciences, Kiev, U.S.S.R.
Abstract:
The origin of cylindrically-symmetric supernova remnants is discussed. The results of numerical simulations of two most distinguished barrel-like remnants SNR 1006 and G296.5+10.0 are presented.