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dc.contributor.authorHinton, J. A.-
dc.contributor.authorPope, E. C. D.-
dc.contributor.authorDomainko, W.-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2007, 382 (1), pp. 466-472-
dc.description.abstractRecent observations have revealed the existence of enormously energetic ∼1061 erg active galactic nuclei outbursts in three relatively distant galaxy clusters. These outbursts have produced bubbles in the intracluster medium, apparently supported by pressure from relativistic particles and/or magnetic fields. Here, we argue that if ≥GeV particles are responsible then these particles are very likely protons and nuclei, rather than electrons, and that the γ-ray emission from these objects, arising from the interactions of these hadrons in the intracluster medium, may be marginally detectable with instruments such as the Gamma-ray Large Area Space Telescope (GLAST) and the High Energy Stereoscopic System (HESS).-
dc.publisherRoyal Astronomical Society (RAS)-
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2007 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.-
dc.titleγ-ray emission associated with cluster-scale AGN outbursts-
dc.typeJournal Article-
dc.description.versionPublisher Version-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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