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Multiple simultaneous Gamma-ray emission sites in 3C 84

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arxiv 1612.07874 v1 pith:KHCXSUXP submitted 2016-12-23 astro-ph.HE

Jeffrey A. Hodgson , S.S. Lee , B. Rani , J.C. Algaba This is my paper
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keywords emissionbrightfeaturegammagamma-raymovingnearoriginates
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abstract

The mis-aligned active galactic nuclei (AGN), 3C\,84, has been observed approximately monthly at four frequencies simultaneously (22\,GHz -- 129\,GHz) on the Korean VLBI Network (KVN) since 2013 as part of the interferometric monitoring of $\gamma$-ray bright AGN (iMOGABA) program. 3C\,84 is known to have to sites of bright radio emission, with the first thought to be near the central super-massive black hole and the second in a slowly moving emission feature, several milliarcseconds south of the core. Analysis of this data suggests that the highly variable Gamma-ray emission originates near the SMBH and the slowly rising $\gamma$-ray emission originates in the slow moving feature.

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