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

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.

Object Details

• Location: Deutsche Nationalbibliothek Frankfurt am Main
• Extent: Online-Ressource
• Language: Englisch

References and Relationships

• Bibliographic citation: Features of globular cluster’s dynamics with an intermediate-mass black hole ; volume:27 ; number:1 ; year:2018 ; pages:1-6 ; extent:6 ; Open astronomy ; 27, Heft 1 (2018), 1-6 (gesamt 6)

Contributors, Places and Time

• Creator: Ryabova, Marina V. ; Gorban, Alena S. ; Shchekinov, Yuri A. ; Vasiliev, Evgenii O.

Further information

• DOI: 10.1515/astro-2018-0001
• URN: urn:nbn:de:101:1-2405281610224.524845623807
• Rights: Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
• Last update: 14.08.2025, 10:45 AM CEST