Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments
Abstract. We model the inspiral of globular clusters (GCs) towards a galactic nucleus harbouring a supermassive black hole (SMBH), a leading scenario for the f
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 April 16
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 477, Heft: 4, Pages: 4423-4442 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty922 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty922 Verlag, Volltext: https://academic.oup.com/mnras/article/477/4/4423/4972778 
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| Verfasserangaben: | Manuel Arca-Sedda and Alessia Gualandris |
| Zusammenfassung: | Abstract. We model the inspiral of globular clusters (GCs) towards a galactic nucleus harbouring a supermassive black hole (SMBH), a leading scenario for the f |
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| Beschreibung: | Gesehen am 05.02.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty922 |