Can GLAST detect gamma-rays from the extended radio features of radio galaxies?

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dc.creatorSambruna, R. M.
dc.creatorGeorganopoulos, M.
dc.creatorDavis, D.
dc.creatorCillis, A.
dc.date2007-04-09
dc.date.accessioned2026-07-07T07:55:45Z
dc.date.available2026-07-07T07:55:45Z
dc.descriptionA few FRI radio galaxies were detected at GeV gamma-rays with CGRO EGRET, with peroperties suggesting that the gamma-ray flux originates from the core. Here we discuss the possibility that the extended radio features of radio galaxies could be detected with the LAT, focusing on the particularly promising case of the nearby giant radio galaxy Fornax A.
dc.descriptionProceedings of the First GLAST Symposium, February 2007, Stanford, CA
dc.identifierhttps://arxiv.org/abs/0704.1112
dc.identifierhttp://arxiv.org/abs/0704.1112
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/127075
dc.subjectAstrophysics
dc.titleCan GLAST detect gamma-rays from the extended radio features of radio galaxies?
dc.typetext

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