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Partial tidal disruption events by intermediate-mass black holes in supermassive and intermediate-mass black hole binaries

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成果类型:
期刊论文
作者:
Wu, Xiao-Jun;Yuan, Ye-Fei;Luo, Yan;Lin, Wenbin
通讯作者:
Lin, WB;Yuan, YF
作者机构:
[Lin, Wenbin; Wu, Xiao-Jun; Lin, WB] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
[Wu, Xiao-Jun] Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.
[Yuan, Ye-Fei; Luo, Yan] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China.
[Yuan, Ye-Fei; Luo, Yan] Univ Sci & Technol China, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China.
[Lin, Wenbin; Lin, WB] Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Peoples R China.
通讯机构:
[Yuan, YF ; Lin, WB ] U
Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China.
Univ Sci & Technol China, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China.
Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Peoples R China.
语种:
英文
关键词:
methods: numerical;stars: kinematics and dynamics;Galaxy: centre;Galaxy: kinematics and dynamics;transients: tidal disruption events
期刊:
Monthly Notices of the Royal Astronomical Society
ISSN:
0035-8711
年:
2024
卷:
529
期:
2
页码:
1440-1449
基金类别:
National Natural Science Foundation of China [12393812, 11973025]; National Natural Science Foundation of China [2020SKA0120300]; National SKA Program of China [XDB0550200]; Strategic Priority Research Program of the Chinese Academy of Sciences
机构署名:
本校为第一且通讯机构
院系归属:
核科学技术学院
数理学院
摘要:
In the centres of galaxies, stars that orbit supermassive black hole binaries (SMBHBs) can undergo tidal disruptions due to the Lidov–Kozai mechanism. Nevertheless, most previous researches have predominantly focused on full tidal disruption events (FTDEs). In this study, we employ N-body simulations to investigate partial tidal disruption events (PTDEs) induced by intermediate-mass black holes (IMBHs) in SMBH–IMBH binaries, taking into account consideration the IMBH’s mass, semimajor axis, and eccentricity of the outer orbit. Our findings i...

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