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Supermassive black holes coalescence mediated by massive perturbers: implications for gravitational waves emission and nuclear cluster formation

ABSTRACT. A large fraction of galactic nuclei is expected to host supermassive black hole binaries (BHB), likely formed during the early phase of galaxies asse

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Bibliographic Details
Main Authors: Arca Sedda, Manuel (Author) , Berczik, Peter (Author) , Spurzem, Rainer (Author)
Format: Article (Journal)
Language:English
Published: 2019
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 484, Issue: 1, Pages: 520-542
ISSN:1365-2966
DOI:10.1093/mnras/sty3458
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty3458
Verlag, Volltext: https://academic.oup.com/mnras/article/484/1/520/5253622
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Author Notes:Manuel Arca Sedda, Peter Berczik, Roberto Capuzzo-Dolcetta, Giacomo Fragione, Margaryta Sobolenko and Rainer Spurzem
Description
Summary:ABSTRACT. A large fraction of galactic nuclei is expected to host supermassive black hole binaries (BHB), likely formed during the early phase of galaxies asse
Item Description:Gesehen am 15.02.2019
Advance access publication 2018 December 19
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty3458

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