Relativistic Outflow Drives γ-Ray Emission in 3C 345
J. Anton ZensusMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
2011en
ABI
Annotatsiya
Aims. On the basis of the first 20 months of Fermi-LAT data and optical monitoring, the quasar 3C 345 has been identified as a γ-ray emitter. We investigate whether there is a connection between the γ-ray and optical variability of 3C 345 and the properties of its parsec-scale radio emission.
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