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Volume 344 - 14th European VLBI Network Symposium & Users Meeting (EVN2018) - AGN Session 1
Does Cygnus A harbor a binary super-massive black hole?
U. Bach,* B. Boccardi, T.P. Krichbaum, A. Lobanov
*corresponding author
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Pre-published on: 2019 March 26
Published on: 2019 October 09
Recently a new radio source was detected with the VLA close to Cygnus A at a distance of about 460 parsec from the center of the AGN. The source is not directly associated with the VLBI core and the jets, but coincides with a compact optical/near-IR source. We detected the new source on sub-parsec scales with EVN observations at 1.3 cm in March 2017 and 6 cm in June 2017. It appears nearly point-like and more luminous than any known radio super-nova. The most plausible origin of the emission is a recent onset of activity from a so far not detected secondary super-massive black hole (SMBH). It could be an extreme type of a super-nova, but the enormous luminosity and compactness on sub-parsec scales and the flat spectral index suggest that a secondary SMBH may exist in the immediate surroundings of the central engine in Cygnus A. Here we present our EVN observations and discuss their implications.
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