Variability of Hard Gamma Ray Emission from Active Galaxies Observed by EGRET

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Session 44 -- Radio Galaxies, Jets and Disks
Display presentation, Wednesday, 9:20-6:30, Pauley Room

[44.09] Variability of Hard Gamma Ray Emission from Active Galaxies Observed by EGRET

P. Michelson, J. Chiang, Y. C. Lin, P. L. Nolan (Stanford), D. L. Bertsch, B. L. Dingus, C. E. Fichtel, R. C. Hartman, S. D. Hunter, J. R. Mattox, P. Sreekumar, D. J. Thompson (NASA/GSFC), K. Brazier, G. Kanbach, H. A. Mayer-Hasselwander, C. von Montigny (MPE), D. A. Kniffen (Hampden-Sydney College), E. J. Schneid (Grumman)

During approximately the first 18 months of the Compton Observatory mission, the EGRET telescope has detected more than 20 active galaxies that are predominantly flat-spectrum radio-loud quasars. Temporal variability of the gamma-ray flux is observed in many of these sources. A summary of these observations is presented along with discussion of the implications for emission models.

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