Cosmic rays from supernova remnants and superbubbles

被引：19
|
作者：
Lingenfelter, Richard E. [1 ]
机构：
[1] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
来源：
ADVANCES IN SPACE RESEARCH | 2018年 / 62卷 / 10期
关键词：
Cosmic rays; Shock acceleration; Superbubbles; Supernova remnants; INTERSTELLAR-MEDIUM; OB ASSOCIATIONS; STAR-FORMATION; PARTICLE-ACCELERATION; ELEMENTS FE-26; MASSIVE STARS; IC; 443; ORIGIN; EVOLUTION; ABUNDANCES;
D O I：
10.1016/j.asr.2017.04.006
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Recent high energy gamma-ray observations of both single supernova remnants and superbubbles, together with observations of supernovae, star formation regions, and local cosmic ray composition, now provide an integrated framework tying together the sources, injection, acceleration, and propagation of the cosmic rays, so that it is possible to determine their relative contributions to cosmic ray acceleration for all but the very highest energies. (C) 2017 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码：2750 / 2763
页数：14
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