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Home Search Quick Search Advanced Fulltext Browse Collections Persons My eDoc Login Name: Password: Documentation Help Support Wiki Direct access to document ID:	Document History for Document ID 318865.0 Back to latest document version Document Version Version Comment Date Status 318865.0 [No comment] 09.02.2009 09:53 Released 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 Full Text: You have privileges to view the following file(s): eDoc318865arxiv.pdf  [186,00 Kb] [Comment:arXiv:astro-ph/0310276]