ON NONTHERMAL PARTICLE GENERATION IN SUPERBUBBLES

被引：105

作者：

BYKOV, AM

FLEISHMAN, GD

机构：

[1] A.F. Loffe Institute of Physics and Technology, Academy of Sciences, St Petersburg

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1992年 / 255卷 / 02期

关键词：

D O I：

10.1093/mnras/255.2.269

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Generation of non-thermal particles in an OB association is studied. A model of cosmic-ray acceleration is proposed where the interaction of charged particles with an ensemble of shocks and large-scale plasma motions inside the bubble is included. The cosmic-ray acceleration appears to be very efficient especially after explosions of a few supernovae in the association. The cosmic-ray acceleration time is of the order of 10(5) yr. Some tens of per cent of the bubble kinetic energy can be converted to the cosmic-ray acceleration.

引用

页码：269 / 275

页数：7

共 24 条

[11] SUPERNOVAE VERSUS MODELS OF THE INTERSTELLAR-MEDIUM AND THE GASEOUS HALO [J].