Limits to extragalactic cosmic rays from gamma-ray fluxes
- 1 March 1982
- journal article
- Published by IOP Publishing in Journal of Physics G: Nuclear Physics
- Vol. 8 (3) , 383-391
- https://doi.org/10.1088/0305-4616/8/3/009
Abstract
Models involving the production of cosmic-ray protons and heavier nuclei of energies in the range 1-10 GeV in extragalactic space are considered and the fluxes of gamma rays expected from their interactions with gas in clusters of galaxies are derived. Comparison with observation allows limits to be set on the fraction of the cosmic-ray flux detected at the Earth which is derived from extragalactic sources. It is found that for all reasonable models of extragalactic origin an excess of gamma -ray flux would result; thus, the bulk of the 1-10 GeV cosmic rays detected appear to be of Galactic origin.Keywords
This publication has 21 references indexed in Scilit:
- Ultra-high-energy cosmic rays from clusters of galaxiesJournal of Physics G: Nuclear Physics, 1980
- X-ray measurements of the mass of M87The Astrophysical Journal, 1980
- The diffuse X-ray background spectrum from 3 to 50 keVThe Astrophysical Journal, 1980
- X-ray observations of galaxies in the Virgo clusterThe Astrophysical Journal, 1979
- Measurements of the gas contents of clusters of galaxies by observations of the background radiation at 10.6 GHzMonthly Notices of the Royal Astronomical Society, 1978
- The detection of large X-ray halos in clustersThe Astrophysical Journal, 1978
- Thermal-Bremsstrahlung Interpretation of Cluster X-Ray SourcesThe Astrophysical Journal, 1973
- Density Data and Emission Measure for a Model of the Coma ClusterThe Astrophysical Journal, 1972
- Active Galaxies with Radio Trails in ClustersNature, 1972
- The Distribution of Rich Clusters of Galaxies.The Astrophysical Journal Supplement Series, 1958