Features of globular cluster’s dynamics with an intermediate-mass black hole

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DC Field	Value	Language
dc.contributor.author	Ryabova, M V	-
dc.contributor.author	Gorban, Alena S	-
dc.contributor.author	Shchekinov, Yuri	-
dc.contributor.author	Vasiliev, Evgenii O.	-
dc.date.accessioned	2018-05-28T16:19:39Z	-
dc.date.available	2018-05-28T16:19:39Z	-
dc.date.issued	2018-02	-
dc.identifier.citation	Open Astronomy, 2018, Vol. 27, p1-6	en_US
dc.identifier.issn	2543-6376	-
dc.identifier.uri	http://hdl.handle.net/2289/6915	-
dc.description	Open Access	en_US
dc.description.abstract	In this paper, we address the question of how a central intermediate-mass black hole (IMBH) in a globular cluster (GC) affects dynamics, core collapse, and formation of the binary population. It is shown that the central IMBH forms a binary system that affects dynamics of stars in the cluster significantly. The presence of an intermediate-mass black hole with mass ≥ 1.0-1.7%of the total stellar mass in the cluster inhibits the formation of binary stars population.	en_US
dc.language.iso	en	en_US
dc.publisher	De Gruyter	en_US
dc.relation.uri	http://adsabs.harvard.edu/abs/2018OAst...27....1R	en_US
dc.relation.uri	https://doi.org/10.1515/astro-2018-0001	en_US
dc.rights	2018 M V Ryabova et al	en_US
dc.subject	star Clusters	en_US
dc.subject	black	en_US
dc.title	Features of globular cluster’s dynamics with an intermediate-mass black hole	en_US
dc.type	Article	en_US
Appears in Collections:	Research Papers (A&A)

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