The MEGaN project: I. Missing formation of massive nuclear clusters and tidal disruption events by star clusters-massive black hole interactions

We investigated the evolution of a massive galactic nucleus hosting a supermassive black hole (SMBH) with mass MSMBH = 108 M ⊙ surrounded by a population of 42 heavy star clusters (globular clusters, GCs). Using direct N-body modelling, we show here that the assembly of a nuclear star cluster (NSC)...

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Bibliographic Details
Main Authors: Arca Sedda, Manuel (Author) , Capuzzo-Dolcetta, Roberto (Author)
Format: Article (Journal)
Language:English
Published: 26 June 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 471, Issue: 1, Pages: 478-490
ISSN:1365-2966
DOI:10.1093/mnras/stx1586
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx1586
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Author Notes:M. Arca-Sedda and R. Capuzzo-Dolcetta
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The MEGaN project: I. Missing formation of massive nuclear clusters and tidal disruption events by star clusters - massive black hole interactions by Arca Sedda, Manuel (Author) , Capuzzo-Dolcetta, Roberto (Author) ,


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