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Radio Flaring Activity of 3C 345 and its Connection to Gamma-ray Emission

3C 345 is one of the archetypical active galactic nuclei, showing structural and flux variability on parsec scales near a compact unresolved radio core. During the last 2 years, the source has been undergoing a period of high activity visible in the broad spectral range, from radio through high-energy bands. We have been monitoring parsec-scale radio emission in 3C 345 during this period at monthly intervals, using the VLBA at 15, 24, and 43 GHz. Our radio observations are compared with gamma-ray emission detected by Fermi-LAT in the region including 3C 345 (1FGL J1642.5+3947). Three distinct gamma-ray events observed in this region are associated with the propagation of relativistic plasma condensations inside the radio jet of 3C 345. We report on evidence for the gamma-rays to be produced in a region of the jet of up to 40 pc (de-projected) in extent. This suggests the synchrotron self-Compton process as the most likely mechanism for production of gamma-rays in the source.

preprint2010arXivOpen access
F. K. SchinzelA. P. LobanovS. G. JorstadA. P. MarscherG. B. TaylorJ. A. Zensus
astro-ph.GAastro-ph.HE
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F. K. SchinzelA. P. LobanovS. G. JorstadA. P. MarscherG. B. TaylorJ. A. Zensus

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