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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| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2019
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 484, Heft: 1, Pages: 520-542 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty3458 |
| Online-Zugang: | 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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| Verfasserangaben: | Manuel Arca Sedda, Peter Berczik, Roberto Capuzzo-Dolcetta, Giacomo Fragione, Margaryta Sobolenko and Rainer Spurzem |
| Zusammenfassung: | 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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| Beschreibung: | Gesehen am 15.02.2019 Advance access publication 2018 December 19 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty3458 |