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

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dc.contributor.advisor Jenet, F. A. en_US
dc.contributor.author Lommen, A. en_US
dc.contributor.author Larson, S. L. en_US
dc.contributor.author Wen, L. en_US
dc.date.accessioned 2004-11-10T16:03:02Z
dc.date.available 2004-11-10T16:03:02Z
dc.date.issued 2003
dc.identifier.citation Astrophysical journal, vol.606, pp.799-803 en_US
dc.identifier.clearanceno 03-2782
dc.identifier.uri http://hdl.handle.net/2014/37352
dc.description.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. en_US
dc.format.extent 180301 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other pulsars en_US
dc.subject.other gravitational waves en_US
dc.subject.other black holes en_US
dc.title Constraining the properties of the proposed supermassive black hole system in 3C66B: limits from pulsar timing en_US


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