Cosmic ray ions, dust and the interstellar medium

被引：0
|
作者：
Erlykin, AD
Wolfendale, AW
机构：
[1] PN Lebedev Phys Inst, Moscow 117924, Russia
[2] Univ Durham, Dept Phys, Durham DH1 3LE, England
来源：
PHYSICA SCRIPTA | 2001年 / T95卷
关键词：
D O I：
10.1238/Physica.Topical.095a00092
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The origin of cosmic rays is a continuing problem in Astrophysics. The majority appear to be of Galactic origin and the manner of acceleration seems to involve ions from the ISM being accelerated by shocks from supernova remnants. Dust in the ISM may also play a part in the early stages. The paper gives a brief account of the origin problem and the likely acceleration mechanisms.
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页码：92 / 95
页数：4
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