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Radio evidence for binary super massive black holes
2014
Proceedings of the International Astronomical Union
Preserved Fulltext
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.
doi:10.1017/s1743921315007401
fatcat:vr52urw6krdpbbtx7jiuh3aa2a