Interaction of a Supernova Shock with the other Star in a Binary System

Interaction of a fast shock wave generated during a supernova explosion with a magnetized star-companion of the supernova precursor produces a current sheet. We consider the evolution of this current sheet and show that a singularity (shock) is formed in finite time within the ideal MHD framework. Charged particles (electrons) are accelerated in the vicinity of the singularity, and their distribution function has a plateau up to the energies of the order of ${10}^{4}m{c}^2$. These fast particles radiate in the $\gamma$-range in the strong magnetic field of the current sheet ($B\simeq {10}^{6}G$). Radiation is concentrated within a narrow angle around the current sheet, $\Delta\theta \simeq 3\cdot 10^{-4}$,anditsspectrumhasthemaximumatseveralhundredsof$keV$. Presented calculations confirm the model of cosmological GRBs proposed by Istomin & Komberg (2002).