Pulsar Timing Arrays and the Challenge of Massive Black Hole Binary Astrophysics-Reference-Cited by-同舟云学术

Pulsar Timing Arrays and the Challenge of Massive Black Hole Binary Astrophysics

Published:2014-11-10 Issue: Volume: Page:147-165
ISSN:1570-6591
Container-title:Gravitational Wave Astrophysics
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Author:

Sesana A.

Publisher

Springer International Publishing

Link

http://link.springer.com/content/pdf/10.1007/978-3-319-10488-1_13

Reference70 articles.

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2. P.J. Armitage, P. Natarajan, Eccentricity of supermassive black hole binaries coalescing from gas-rich mergers. Astrophys. J. 634, 921–927 (2005)

3. Z. Arzoumanian et al., NANOGrav limits on gravitational waves from individual supermassive black hole binaries in circular orbits. ArXiv e-prints (April 2014)

4. S. Babak, A. Sesana, Resolving multiple supermassive black hole binaries with pulsar timing arrays. Phys. Rev. D 85(4), 044034 (2012)

5. S. Burke-Spolaor, Multi-messenger approaches to binary supermassive black holes in the continuous-wave regime. Class. Quantum Grav. 30(22), 224013 (2013)

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