Test of Galactic Cosmic-Ray source models - Working group report

被引：49

作者：

Drury, LO ^{[1
]}

Ellison, DE

Aharonian, FA

Berezhko, E

Bykov, A

Decourchelle, A

Diehl, R

Meynet, G

Parizot, E

Raymond, J

Reynolds, S

Spangler, S

机构：

[1] Dublin Inst Adv Studies, IRL, Dublin 2, Ireland

[2] N Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA

[3] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[4] Inst Cosmophys Res & Aeron, Yakutsk 677891, Russia

[5] AF Ioffe Phys Tech Inst, St Petersburg 194021, Russia

[6] CEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, France

[7] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany

[8] Observ Geneva, CH-1290 Sauverny, Switzerland

[9] Inst Phys Nucl, F-91406 Orsay, France

[10] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[11] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA

来源：

SPACE SCIENCE REVIEWS | 2001年 / 99卷 / 1-4期

关键词：

D O I：

10.1023/A:1013825905795

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The main features of cosmic-ray source models and acceleration processes are reviewed, with special emphasis on the possible observational tests, through both composition analysis and multi-wavelength studies of supernova remnants. Non-linear effects in the context of supernova-induced diffusive shock acceleration are discussed, as well as collective acceleration effects induced by multiple supernova explosions inside superbubbles.

引用

页码：329 / 352

页数：24

共 102 条

[1]

ACHTERBERG A, 1994, ASTRON ASTROPHYS, V281, P220

[2] Evidence of X-ray synchrotron emission from electrons accelerated to 40 TeV in the supernova remnant Cassiopeia A [J].