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  Constraining the Properties of the Proposed Super-Massive Black Hole System in 3C66B: Limits from Pulsar Timing

Jenet, F., Lommen, A., Larson, S. L., & Wen, L. (2005). Constraining the Properties of the Proposed Super-Massive Black Hole System in 3C66B: Limits from Pulsar Timing. In F. A. Rasio, & I. H. Stairs (Eds.), Binary radio pulsars: proceedings of a meeting held in Aspen, Colorado, USA 11-17 January 2004 (pp. 399). San Francisco, Calif.: Astronomical Soc. of the Pacific.

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eDoc318865arxiv.pdf (Preprint), 187KB
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eDoc318865arxiv.pdf
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 Creators:
Jenet, F.A., Author
Lommen, A., Author
Larson, Shane L., Author
Wen, L.1, Author
Affiliations:
1Theoretical Gravitational Wave Physics, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24015              

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 Dates: 2005
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 318865
Other: arXiv:astro-ph/0310276
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Title: Binary radio pulsars
Place of Event: Aspen, Colorado, USA
Start-/End Date: 2004-01-11 - 2004-01-17

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Title: Binary radio pulsars : proceedings of a meeting held in Aspen, Colorado, USA 11-17 January 2004
Source Genre: Proceedings
 Creator(s):
Rasio, F. A., Editor
Stairs, I. H., Editor
Affiliations:
-
Publ. Info: San Francisco, Calif. : Astronomical Soc. of the Pacific
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 399 Identifier: -

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Title: Astronomical Society of the Pacific conference series
Source Genre: Series
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Pages: - Volume / Issue: 328 Sequence Number: - Start / End Page: - Identifier: -