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  Galaxy mergers and implications for massive black hole binary coalescence

Vecchio, A. (1997). Galaxy mergers and implications for massive black hole binary coalescence. Classical and Quantum Gravity, 14(6), 1431-1437. doi:10.1088/0264-9381/14/6/007.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5A98-6 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5A99-4
Genre: Journal Article

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 Creators:
Vecchio, Alberto1, 2, Author
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24010              
2AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24009              

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 Abstract: Massive black hole binaries are one of the most interesting classes of sources that could be detectable by LISA, as they allow tests of general relativity in strong-field conditions and to probe into the very centre of galactic nuclei. We review our present knowledge about the scenario that leads to the formation of these systems and the event rate of detectable gravitational wave signals. We also discuss the use of a LISA-observation catalogue to gain information on the mass - redshift distribution of sources.

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Language(s): eng - English
 Dates: 1997-06
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Method: -
 Identifiers: eDoc: 328679
ISI: A1997XF50700007
DOI: 10.1088/0264-9381/14/6/007
 Degree: -

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Title: Classical and Quantum Gravity
  Alternative Title : Class. Quantum Gravity
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 14 (6) Sequence Number: - Start / End Page: 1431 - 1437 Identifier: ISSN: 0264-9381