Supernova Remnants as Sources of Cosmic Rays and Nonthermal Emission


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

Cosmic ray acceleration by astrophysical shocks in supernova remnants is briefly reviewed. Results of numerical modeling taking into account magnetic field amplification by streaming instability and shock modification are presented. Nonthermal emission produced by accelerated particles in young and old supernova remnants is compared with available data of radio, X-ray, and gamma-ray astronomy. We also discuss a possibility of particle acceleration to PeV energies at supernova shocks propagating in the interstellar bubbles created by stellar winds of supernova progenitors.

作者简介

V. Zirakashvili

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

编辑信件的主要联系方式.
Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840

V. Ptuskin

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2019