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Constraining the properties of the proposed supermassive black hole system in 3C66B: limits from pulsar timingData 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.
Document ID
20060042596
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Jenet, F. A.
Lommen, A.
Larson, S. L.
Wen, L.
Date Acquired
August 23, 2013
Publication Date
January 1, 2003
Publication Information
Publication: Astrophysical Journal
Volume: 606
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
pulsars
black holes
gravitational waves

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