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Radio evidence for binary super massive black holes

Published online by Cambridge University Press:  07 March 2016

R. D. Ekers
R. D. Ekers*
Affiliation:
CSIRO Astronomy and Space Vimera and Pembroke Roads, Marsfield, NSW 2122, Australia email: ron.ekers@csiro.au
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Abstract

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I present examples of radio AGN with binary nuclei which provide the direct radio evidence for binary Super Massive Black Holes (SMBH) driving the AGN activity. There is also other evidence for distorted radio morphology and periodic variability which may indicate the presence of a second (inactive) SMBH. Finally I enumerate a number of possible radio tracers for the binary SMBH merger events.

Keywords

Super Massive Black Holes (SMBH)binaryAGN
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S312: Star Clusters and Black Holes in Galaxies across Cosmic Time , August 2014 , pp. 26 - 30
Copyright
Copyright © International Astronomical Union 2016 

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