Speaker
Vladimir Zirakashvili
(Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Moscow, Russia)
Description
Diffusive shock acceleration and production of non-thermal emission in galactic supernova remnants is briefly reviewed. We describe gamma ray and X-ray observational features of young and old remnants. The corresponding discussion of Galactic cosmic ray origin is given.
Primary author
Vladimir Zirakashvili
(Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Moscow, Russia)
