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

Lommen, A.; Larson, S. L.; Wen, L.

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