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Planetary systems in a star cluster II: intermediate-mass black holes and planetary systems

ABSTRACT. Most stars form in dense stellar environments. It is speculated that some dense star clusters may host intermediate-mass black holes (IMBHs), which m

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Bibliographic Details
Main Authors: Flammini Dotti, Francesco (Author) , Kouwenhoven, M. B. N. (Author) , Shu, Qi (Author) , Hao, Wei (Author) , Spurzem, Rainer (Author)
Format: Article (Journal)
Language:English
Published: 2020 July 27
In: Monthly notices of the Royal Astronomical Society
Year: 2020, Volume: 497, Issue: 3, Pages: 3623-3637
ISSN:1365-2966
DOI:10.1093/mnras/staa2188
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa2188
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/497/3/3623/5876890
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Author Notes:Francesco Flammini Dotti, M.B.N. Kouwenhoven, Qi Shu, Wei Hao and Rainer Spurzem
Description
Summary:ABSTRACT. Most stars form in dense stellar environments. It is speculated that some dense star clusters may host intermediate-mass black holes (IMBHs), which m
Item Description:Gesehen am 11.11.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/staa2188

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