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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

Lommen, A.; Larson, S. L.; Wen, L.
URI: http://hdl.handle.net/2014/37352
Date: 2003
Citation: Astrophysical journal, vol.606, pp.799-803

Abstract:

Data from long term timing observations of the radio pulsar PSR B1855+09 have been searched for the signature of Gravitational waves (G-waves) emitted by the proposed supermassive binary black hole system in 3C66B.

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