English
 
User Manual Privacy Policy Disclaimer Contact us
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Conference Paper

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

MPS-Authors

Wen,  L.
Theoretical Gravitational Wave Physics, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

External Ressource
No external resources are shared
Fulltext (public)

eDoc318865arxiv.pdf
(Preprint), 187KB

Supplementary Material (public)
There is no public supplementary material available
Citation

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.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0013-4FA6-0
Abstract
There is no abstract available