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