On the spectrum of high-energy cosmic rays produced by supernova remnants in the presence of strong cosmic-ray streaming instability and wave dissipation
- 5 January 2005
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 429 (3) , 755-765
- https://doi.org/10.1051/0004-6361:20041517
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
All Related Versions
This publication has 32 references indexed in Scilit:
- Extragalactic UHE proton spectrum and prediction for iron-nuclei flux at 108–109 GeVAstroparticle Physics, 2004
- Cosmic ray production in supernova remnants including reacceleration: The secondary to primary ratioAstronomy & Astrophysics, 2003
- A search for TeV gamma-ray emission from SNRs, pulsars and unidentified GeV sources in the Galactic plane in the longitude range between $-2^\circ$ and $85^\circ$Astronomy & Astrophysics, 2002
- A model of particle acceleration to high energies by multiple supernova explosions in OB associationsAstronomy Letters, 2001
- Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic fieldMonthly Notices of the Royal Astronomical Society, 2001
- Shock-wave propagation in the nonuniform interstellar mediumReviews of Modern Physics, 1995
- The origins of high-energy cosmic raysThe Astrophysical Journal Supplement Series, 1994
- Acceleration of cosmic rays by shock wavesSoviet Physics Uspekhi, 1988
- Supernova shock acceleration of cosmic rays in the GalaxyThe Astrophysical Journal, 1980
- The acceleration of cosmic rays in shock fronts - IMonthly Notices of the Royal Astronomical Society, 1978