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Gamma‐rays from 3C279 and universal energy spectrum
dc.contributor.authorTomozawa, Yukioen_US
dc.date.accessioned2011-11-15T15:58:47Z
dc.date.available2011-11-15T15:58:47Z
dc.date.issued1992-05-01en_US
dc.identifier.citationTomozawa, Yukio (1992). "Gamma‐rays from 3C279 and universal energy spectrum." AIP Conference Proceedings 254(1): 345-347. <http://hdl.handle.net/2027.42/87336>en_US
dc.identifier.otherAPCPCS-254-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87336
dc.description.abstractIt has been suggested that the energy spectrum from point sources such as galactic black hole candidates (GBHC) and active galactic nuclei (AGN) is universal on the average. Recent measurements of γ‐rays from 3C279 by the EGRET detector of Compton Observatory (alias GRO) are discussed and compared with the source spectrum of cosmic rays.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleGamma‐rays from 3C279 and universal energy spectrumen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumRandall Laboratory of Physics, University of Michigan, Ann Arbor, Michigan 48109‐1120en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87336/2/345_1.pdf
dc.identifier.doi10.1063/1.42210en_US
dc.identifier.sourceTesting the AGN paradigmen_US
dc.owningcollnamePhysics, Department of


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