Constraining the properties of the proposed supermassive black hole system in 3C66B: Limits from pulsar timing

Details Constraining the properties of the proposed supermassive black hole system in 3C66B: Limits from pulsar timing Constraining the properties of the proposed supermassive black hole system in 3C66B: Limits from pulsar timing

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20310402j&link_type=abstract

American Astronomical Society Meeting 203, #104.02; Bulletin of the American Astronomical Society, Vol. 35, p.1372

Astronomy and Astrophysics

Astronomy

Scientific paper

Using pulsar timing data, limits are placed on the mass and eccentricity of the supermassive binary black hole (SBBH)system in 3C66B recently proposed by Sudou, Iguchi, Murata, & Taniguchi (2003). The proposed system will emit gravitational waves detectable in pulsar timing data. Since no gravitational waves are detected, it is concluded that the ``chirp mass'' of the SBBH must be less than that adopted by Sudou et al. General features of a gravitational wave detection scheme based on radio pulsar timing are also presented.

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