Cosmic Rays and Nonthermal Radiation in Middle-Aged Supernova Remnants

被引:4
|
作者
Zirakashvili, V. N. [1 ]
Ptuskin, V. S. [1 ]
机构
[1] Russian Acad Sci, Pushkov Inst Terr Magnetism Ionosphere & Radio Wa, Troitsk 108840, Moscow Oblast, Russia
基金
俄罗斯基础研究基金会;
关键词
supernova remnants; interstellar medium; cosmic rays; gamma rays; DIFFUSIVE SHOCK ACCELERATION; STREAMING INSTABILITY; AMPLIFICATION; SIMULATIONS; EMISSION; W28; W44;
D O I
10.1134/S1063773718120071
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A nonlinear model of cosmic-ray acceleration at the shock fronts in the supernova remnants W28, W44, and IC433 is investigated. The hydrodynamic evolution of a supernova remnant, including the shock modification by the pressure of accelerated particles and the streaming instability of particles upstream of the shock propagating in a partially ionized interstellar gas, is modeled. The electromagnetic radiation generated by accelerated particles is calculated and compared with observations in a wide range of photon energies.
引用
收藏
页码:769 / 776
页数:8
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