Parsec-scale Jet Behavior Of The Quasar 3c273 During The High Gamma-ray State In 2009-2010

Astronomy and Astrophysics – Astronomy

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Scientific paper

We analyze total and polarized intensity images of the quasar 3C273 obtained at 43 GHz monthly during 2008-2010 within the Boston U. monitoring program of gamma-ray blazars with the VLBA. We find a strong increase of activity in the parsec-scale jet of the quasar during a high gamma-ray state lasting from 2009 June to 2010 May that features an increase of the total and polarized flux in the mm-wave core and the appearance of superluminal knots in the jets. Although the optical variability is low, owing to strong contamination by the big blue bump, we observe a significant increase in the degree of optical polarization, by a factor of 3, that coincides with a gamma-ray flare in 2010 April. We discuss the locations in the jet where high gamma-ray fluxes occur. These include stationary features in the jet flow that we identify with standing shocks.
This research was supported in part by NASA grants NNX08AV65G, NNX08AV61G, NNX09AT99G, and NNX09AU10G, and NSF grant AST-0907893. The VLBA is an instrument of the National Radio Astronomy Observatory, a facility of the NSF, operated under cooperative agreement by Associated Universities, Inc.

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