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ID: 318865.0, MPI für Gravitationsphysik / Theoretical Gravitational Wave Physics
Constraining the Properties of the Proposed Super-Massive Black Hole System in 3C66B: Limits from Pulsar Timing
Authors:Jenet, F.A.; Lommen, A.; Larson, Shane L.; Wen, L.
Publisher:Astronomical Soc. of the Pacific
Place of Publication:San Francisco, Calif.
Date of Publication (YYYY-MM-DD):2005
Title of Proceedings:Binary radio pulsars : proceedings of a meeting held in Aspen, Colorado, USA 11-17 January 2004
Start Page:399
Title of Series:Astronomical Society of the Pacific conference series
Volume (in Series):328
Name of Conference/Meeting:Binary radio pulsars
Place of Conference/Meeting:Aspen, Colorado, USA
(Start) Date of Conference/Meeting
 (YYYY-MM-DD):
2004-01-11
End Date of Conference/Meeting 
 (YYYY-MM-DD):
2004-01-17
Review Status:not specified
Audience:Not Specified
External Publication Status:published
Document Type:Conference-Paper
Communicated by:Yanbei Chen
Affiliations:MPI für Gravitationsphysik/Theoretical Gravitational Wave Physics
Identifiers:LOCALID:arXiv:astro-ph/0310276
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