The distinction between gamma-quanta spectra from both local sources and cosmic rays, and the formation of a uniform cosmic ray spectrum
Author:
Publisher
Elsevier BV
Subject
Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics
Reference9 articles.
1. TeV gamma-ray emission from point sources: galactic and extragalactic
2. The Supernova Remnants as the main sources of gamma-quanta with energies more than 1 TeV in our Galactic
3. Cosmic rays of energies in the range 103–105 TeV and higher
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1. Shell-type supernova remnants as sources of cosmic rays;Advances in Space Research;2018-11
2. A synchrotron self-Compton emission model compared with the VHE spectrum of Crab Nebula, Geminga energy spectra and hadronic gamma-rays in the Tycho SNR;Nuclear Physics B - Proceedings Supplements;2009-12
3. Extragalactic Background Light and energy spectra of Active Galactic Nuclei 3c454.3 and 1739+522 with high red shifts;Nuclear Physics B - Proceedings Supplements;2009-12
4. Distant metagalactic sources of very high energy γ rays: 1739 + 522 and 3c454.3;Bulletin of the Russian Academy of Sciences: Physics;2009-05
5. Gamma-emission of very high energy from the metagalactic sources Mkn421, Mkn501, NGC1275 and 3c454.3, 1739+522;Nuclear Physics B - Proceedings Supplements;2008-01
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