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MOCCA-SURVEY data base II - Properties of intermediate mass black holes escaping from star clusters

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cris.lastimport.scopus2024-02-12T20:21:07Z
dc.abstract.enIn this work, we investigate properties of intermediate-mass black holes (IMBHs) that escape from star clusters due to dynamical interactions. The studied models were simulated as part of the preliminary second survey carried out using the MOCCA code (MOCCA-SURVEY Database II), which is based on the Monte Carlo N-body method and does not include gravitational wave recoil kick prescriptions of the binary black hole merger product. We have found that IMBHs are more likely to be formed and ejected in models where both initial central density and central escape velocities have high values. Most of our studied objects escape in a binary with another black hole (BH) as their companion and have masses between 100 and $ m 140 { m ~M}_{odot }$. Escaping IMBHs tend to build-up mass most effectively through repeated mergers in a binary with BHs due to gravitational wave emission. Binaries play a key role in their ejection from the system as they allow these massive objects to gather energy needed for escape. The binaries in which IMBHs escape tend to have very high binding energy at the time of escape and the last interaction is strong but does not involve a massive intruder. These IMBHs gain energy needed to escape the cluster gradually in successive dynamical interactions. We present specific examples of the history of IMBH formation and escape from star cluster models. We also discuss the observational implications of our findings as well as the potential influence of the gravitational wave recoil kicks on the process.
dc.affiliationUniwersytet Warszawski
dc.contributor.authorAskar, Abbas
dc.contributor.authorGiersz, Mirek
dc.contributor.authorMaliszewski, Konrad
dc.contributor.authorRosińska, Dorota
dc.contributor.authorHypki, Arkadiusz
dc.date.accessioned2024-01-25T12:46:23Z
dc.date.available2024-01-25T12:46:23Z
dc.date.copyright2022-06-18
dc.date.issued2022
dc.description.accesstimeBEFORE_PUBLICATION
dc.description.financePublikacja bezkosztowa
dc.description.number4
dc.description.versionORIGINAL_AUTHOR
dc.description.volume514
dc.identifier.doi10.1093/MNRAS/STAC1728
dc.identifier.issn0035-8711
dc.identifier.urihttps://repozytorium.uw.edu.pl//handle/item/112735
dc.identifier.weblinkhttp://adsabs.harvard.edu/abs/2022MNRAS.514.5879M
dc.languageeng
dc.pbn.affiliationastronomy
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.relation.pages5879-5889
dc.rightsOther
dc.sciencecloudnosend
dc.titleMOCCA-SURVEY data base II - Properties of intermediate mass black holes escaping from star clusters
dc.typeJournalArticle
dspace.entity.typePublication