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          Institute: MPI für Kernphysik     Collection: High-Energy Astrophysics     Display Documents

ID: 29243.0, MPI für Kernphysik / High-Energy Astrophysics
Test of Galactic Cosmic-Ray source models - Working group report
Authors:Drury, L. O.; Ellison, D. E.; Aharonian, F. A.; Berezhko, E.; Bykov, A.; Decourchelle, A.; Diehl, R.; Meynet, G.; Parizot, E.; Raymond, J.; Reynolds, S.; Spangler, S.
Date of Publication (YYYY-MM-DD):2001-10
Title of Journal:Space Science Reviews
Journal Abbrev.:Space Sci. Rev.
Issue / Number:1-4
Start Page:329
End Page:352
Review Status:Peer-review
Audience:Experts Only
Abstract / Description: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.
External Publication Status:published
Document Type:Article
Affiliations:MPI für Kernphysik/Group H. J. Völk/High Energy Astrophysics (F. Aharonian)
External Affiliations:Dublin Inst Adv Studies, IRL, Dublin 2, Ireland; Dublin Inst Adv Studies, IRL, Dublin 2, Ireland; N Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA; Inst Cosmophys Res & Aeron, Yakutsk 677891, Russia; AF Ioffe Inst Phys & Technol, St Petersburg 194021, Russia; CEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, France; Max Planck Inst Extraterr Phys, D-85741 Garching, Germany; Observ Geneva, CH-1290 Sauverny, Switzerland; Inst Phys Nucl, F-91406 Orsay, France; Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA; Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
Identifiers:ISI:000173468900028 [ID No:1]
ISSN:0038-6308 [ID No:2]
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