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

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dc.contributor.authorRyabova, M V
dc.contributor.authorGorban, Alena S
dc.contributor.authorShchekinov, Yuri A
dc.contributor.authorVasiliev, Evgenii O
dc.date.accessioned2018-05-28T16:19:39Z
dc.date.available2018-05-28T16:19:39Z
dc.date.issued2018-02
dc.descriptionOpen Accessen_US
dc.description.abstractIn 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.identifier.citationOpen Astronomy, 2018, Vol. 27, p1-6en_US
dc.identifier.issn2543-6376
dc.identifier.urihttp://hdl.handle.net/2289/6915
dc.language.isoenen_US
dc.publisherDe Gruyteren_US
dc.relation.urihttp://adsabs.harvard.edu/abs/2018OAst...27....1Ren_US
dc.relation.urihttps://doi.org/10.1515/astro-2018-0001en_US
dc.rights2018 M V Ryabova et alen_US
dc.subjectstar Clustersen_US
dc.subjectblacken_US
dc.titleFeatures of globular cluster’s dynamics with an intermediate-mass black holeen_US
dc.typeArticleen_US

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