Intergalactic shock acceleration and the cosmic gamma-ray background
- 1 November 2002
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 337 (1) , 199-208
- https://doi.org/10.1046/j.1365-8711.2002.05903.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 65 references indexed in Scilit:
- Evidence for shock acceleration and intergalactic magnetic fields in a large-scale filament of galaxies ZwCl 2341.1+0000New Astronomy, 2002
- X‐Ray Synchrotron Emission from 10–100 TeV Cosmic‐Ray Electrons in the Supernova Remnant SN 1006The Astrophysical Journal, 2001
- XMM-Newton observation of the Coma Galaxy clusterAstronomy & Astrophysics, 2001
- A Simple Model of Nonlinear Diffusive Shock AccelerationThe Astrophysical Journal, 1999
- On the Equipartition of Thermal and Nonthermal Energy in Clusters of GalaxiesThe Astrophysical Journal, 1999
- Clusters of Galaxies as Storage Room for Cosmic RaysThe Astrophysical Journal, 1997
- Evidence of X-Ray Synchrotron Emission from Electrons Accelerated to 40 T[CLC]e[/CLC]V in the Supernova Remnant Cassiopeia AThe Astrophysical Journal, 1997
- Distance to the Coma Cluster and a Value for HO Inferred from Globular Clusters in IC 4051The Astronomical Journal, 1997
- The structure of the Virgo cluster of galaxies from Rosat X-ray imagesNature, 1994
- Particle acceleration at astrophysical shocks: A theory of cosmic ray originPhysics Reports, 1987