Constraining the Properties of the Proposed Super-Massive Black Hole System in 3C66B: Limits from Pulsar Timing

Details Constraining the Properties of the Proposed Super-Massive Black Hole System in 3C66B: Limits from Pulsar Timing Constraining the Properties of the Proposed Super-Massive Black Hole System in 3C66B: Limits from Pulsar Timing

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..328..399j&link_type=abstract

Binary Radio Pulsars, ASP Conference Series, Vol. 328, Proceedings of the conference held 11-17 January, 2004, Aspen, Colorado,

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Recent VLBI observations suggest the presence of a supermassive black hole binary system in the core of the radio galaxy 3C 66B. The proposed system would emit high amplitude, low-frequency gravitational wave radiation. This radiation would induce detectable periodic fluctuations in the arrival times of individual pulses from a radio pulsar. The signature of this radiation was searched for in seven years of timing data from the pulsar PSR B1855+09. No evidence for gravitational waves was detected in this data set and limits were placed on the mass and eccentricity of the proposed system.

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