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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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Bibliographic Details
Main Authors: Arca Sedda, Manuel (Author) , Gualandris, Alessia (Author)
Format: Article (Journal)
Language:English
Published: 2018 April 16
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 477, Issue: 4, Pages: 4423-4442
ISSN:1365-2966
DOI:10.1093/mnras/sty922
Online Access: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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Author Notes:Manuel Arca-Sedda and Alessia Gualandris
Description
Summary: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
Item Description:Gesehen am 05.02.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty922

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