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 super-massive black hole (SMBH) with mass $M_\mathrm{SMBH}=10^8 \mathrm{M}_\odot$ surrounded by a population of 42 heavy star clusters (GCs). Using direct $N$-body modelling, we show here that the assembly of an NSC through GCs or...

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Bibliographic Details
Main Authors: Arca Sedda, Manuel (Author) , Capuzzo-Dolcetta, Roberto (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 2017
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1706.06541
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Author Notes:Manuel Arca-Sedda, Roberto Capuzzo-Dolcetta
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