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Supermassive black holes coalescence mediated by massive perturbers: implications for gravitational waves emission and nuclear cluster formation

文献类型：期刊论文

作者Sedda, Manuel Arca2; Berczik, Peter2,3,4,6; Capuzzo-Dolcetta, Roberto1; Fragione, Giacomo5; Sobolenko, Margaryta6; Spurzem, Rainer2,3,4,7,8
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2019-03-01
卷号484期号:1页码:520-542
关键词black hole physics gravitational waves Galaxy: centre galaxies: nuclei galaxies: star clusters: general
ISSN号0035-8711
DOI10.1093/mnras/sty3458
英文摘要A large fraction of galactic nuclei is expected to host supermassive black hole binaries (BI LB), likely formed during the early phase of galaxies assembly and merging. In this paper, we use a large set of state-of-art numerical models to investigate the interplay between a BIM and a massive star cluster (GCs) driven toward the galactic centre by dynamical friction. Varying the BHB mass and mass ratio and the GC orbit, we show that the reciprocal feedback exerted between GCs and the BHB shapes their global properties. We show that, at GC-to-BHB mass ratios above 0.1, the GC affects notably the BHB orbital evolution, possibly boosting its coalescence. This effect is maximized if the GC moves on a retrograde orbit, and for a nonequal mass BHB. We show that the GC debris dispersed around the galactic nucleus can lead to the formation of a nuclear cluster, depending on the BHB tidal field, and that the distribution of compact remnants resulting from the GC disruption can carry information about the BHB orbital properties. We find that red giant stars delivered by the spiralling GC can be disrupted at a rate of similar or equal to (0.7 - 7) x 10(-7) yr(-1) for BHB masses similar to 10(7)M(circle dot), while tens to hundreds of stars can be possibly observed in the galactic halo as high-velocity stars, with velocities up to similar to 2000 km s(-1), depending on the BHB orbital properties.
WOS关键词HIGH-VELOCITY STARS ; TIDAL DISRUPTION ; GLOBULAR-CLUSTER ; SPIRAL GALAXIES ; GALACTIC-CENTER ; STELLAR ENVIRONMENT ; INFALLING CLOUDS ; BINARIES ; EVOLUTION ; MILKY
资助项目Gauss Centre for Supercomputing e.V. ; German Research Foundation (DFG)[Sonderforschungsbereich SFB 881] ; Alexander von Humboldt foundation ; Federal Ministry for Education and Research ; University of Rome Sapienza[52/2015] ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei[90411] ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Arskin postdoctoral fellowship ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Chinese Academy of Sciences[XDB23040100]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000462293100038
出版者OXFORD UNIV PRESS
资助机构Gauss Centre for Supercomputing e.V. ; Gauss Centre for Supercomputing e.V. ; German Research Foundation (DFG) ; German Research Foundation (DFG) ; Alexander von Humboldt foundation ; Alexander von Humboldt foundation ; Federal Ministry for Education and Research ; Federal Ministry for Education and Research ; University of Rome Sapienza ; University of Rome Sapienza ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Arskin postdoctoral fellowship ; Arskin postdoctoral fellowship ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Gauss Centre for Supercomputing e.V. ; Gauss Centre for Supercomputing e.V. ; German Research Foundation (DFG) ; German Research Foundation (DFG) ; Alexander von Humboldt foundation ; Alexander von Humboldt foundation ; Federal Ministry for Education and Research ; Federal Ministry for Education and Research ; University of Rome Sapienza ; University of Rome Sapienza ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Arskin postdoctoral fellowship ; Arskin postdoctoral fellowship ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Gauss Centre for Supercomputing e.V. ; Gauss Centre for Supercomputing e.V. ; German Research Foundation (DFG) ; German Research Foundation (DFG) ; Alexander von Humboldt foundation ; Alexander von Humboldt foundation ; Federal Ministry for Education and Research ; Federal Ministry for Education and Research ; University of Rome Sapienza ; University of Rome Sapienza ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Arskin postdoctoral fellowship ; Arskin postdoctoral fellowship ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; Gauss Centre for Supercomputing e.V. ; Gauss Centre for Supercomputing e.V. ; German Research Foundation (DFG) ; German Research Foundation (DFG) ; Alexander von Humboldt foundation ; Alexander von Humboldt foundation ; Federal Ministry for Education and Research ; Federal Ministry for Education and Research ; University of Rome Sapienza ; University of Rome Sapienza ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Volkswagen Trilateral Project, Dynamical Mechanisms of Accretion in Galactic Nuclei ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Foreign Postdoctoral Fellowship Program of the Israel Academy of Sciences and Humanities ; Arskin postdoctoral fellowship ; Arskin postdoctoral fellowship ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Lady Davis Fellowship Trust at the Hebrew University of Jerusalem ; Chinese Academy of Sciences ; Chinese Academy of Sciences
源URL[http://ir.bao.ac.cn/handle/114a11/25681]  
专题中国科学院国家天文台
通讯作者Sedda, Manuel Arca
作者单位1.Sapienza Univ Roma, Dept Phys, Ple A Moro 5, I-00185 Rome, Italy
2.Heidelberg Univ, Zentrum Astron, Astron Rechen Inst, Monchhofstr 12-14, D-69120 Heidelberg, Germany
3.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China
4.Chinese Acad Sci, Key Lab Computat Astrophys, 20A Datun Rd, Beijing 100012, Peoples R China
5.Hebrew Univ Jerusalem, Racah Inst Phys, IL-9190401 Jerusalem, Israel
6.Natl Acad Sci Ukraine, Main Astron Observ, 27 Akad Zabolotnoho St, UA-03680 Kiev, Ukraine
7.Peking Univ, Kavli Inst Astron & Astrophys, Yiheyuan Lu 5, Beijing 100871, Peoples R China
8.Frankfurt Inst Adv Study, Frankfurt, Germany
推荐引用方式
GB/T 7714		 Sedda, Manuel Arca,Berczik, Peter,Capuzzo-Dolcetta, Roberto,et al. Supermassive black holes coalescence mediated by massive perturbers: implications for gravitational waves emission and nuclear cluster formation[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,484(1):520-542.
APA Sedda, Manuel Arca,Berczik, Peter,Capuzzo-Dolcetta, Roberto,Fragione, Giacomo,Sobolenko, Margaryta,&Spurzem, Rainer.(2019).Supermassive black holes coalescence mediated by massive perturbers: implications for gravitational waves emission and nuclear cluster formation.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,484(1),520-542.
MLA Sedda, Manuel Arca,et al."Supermassive black holes coalescence mediated by massive perturbers: implications for gravitational waves emission and nuclear cluster formation".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 484.1(2019):520-542.

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