Nonthermal X-rays from supernova remnants

被引：0
|
作者：
Decourchelle, Anne [1 ]
机构：
[1] Univ Paris Diderot, Serv Astrophys, LOrme Merisiers, Lab AIM,CEA,IRFU,CNRS,CEA Saclay, F-91191 Gif Sur Yvette, France
来源：
SUPERNOVA ENVIRONMENTAL IMPACTS | 2014年 / 9卷 / S296期
关键词：
Supernova remnant; Particle acceleration; X-rays; Synchrotron emission; MAGNETIC-FIELD AMPLIFICATION; PARTICLE-ACCELERATION; ELECTRON ACCELERATION; SYNCHROTRON EMISSION; RX J1713.7-3946; COSMIC-RAYS; HIGH-ENERGY; NONLINEAR AMPLIFICATION; SHOCK ACCELERATION; SHELL;
D O I：
10.1017/S174392131300954X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Since the discovery of nonthermal X-rays in the shell-type supernova remnant SN1006 almost 20 years ago, the field has developed considerably, owing significant progress to our understanding of particle acceleration. Key to the characterization of the nonthermal emission is the ability of current satellites, XMM-Newton and Chandra, to perform spatially resolved spectroscopy at a relatively small spatial scale. In this review, I intend to present the main contributions of the study of nonthermal X-rays from supernova remnants to the understanding of particle acceleration.
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收藏
页码：245 / 252
页数：8
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