Does the inverse Compton mechanism alone explain the GeV/TeV gamma-ray emission from the Crab Nebula?
- 1 May 1995
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 3 (3) , 275-282
- https://doi.org/10.1016/0927-6505(95)00006-3
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- Unpulsed high-energy radiation from the Crab pulsar and nebulaThe Astrophysical Journal Supplement Series, 1994
- Observations of the Crab pulsar and nebula by the EGRET telescope on the Compton Gamma-Ray ObservatoryThe Astrophysical Journal, 1993
- The expected high-energy to ultra-high-energy gamma-ray spectrum of the Crab NebulaThe Astrophysical Journal, 1992
- TeV radiation from galactic sourcesSpace Science Reviews, 1992
- Acceleration by pulsar winds in binary systemsThe Astrophysical Journal, 1990
- Magnetohydrodynamic model of Crab nebula radiationThe Astrophysical Journal, 1984
- Confinement of the Crab pulsar's wind by its supernova remnantThe Astrophysical Journal, 1984
- Far-infrared observations of the Crab nebulaThe Astrophysical Journal, 1984
- Production of Cosmic Gamma Rays by Compton Scattering in Discrete SourcesThe Astrophysical Journal, 1969
- High-Energy Photons from the Compton-Synchrotron Process in the Crab NebulaPhysical Review Letters, 1965