中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Cosmic Distributions of Stellar Tidal Disruptions by Massive Black Holes at Galactic Centers

文献类型:期刊论文

作者Chen,Yunfeng2; Yu,Qingjuan2; Lu,Youjun1,3
刊名The Astrophysical Journal
出版日期2020-09-01
卷号900期号:2
ISSN号0004-637X
关键词Astrodynamics Galaxy dynamics Gravitational wave astronomy High energy astrophysics Supermassive black holes Tidal disruption Transient sources Time domain astronomy
DOI10.3847/1538-4357/aba950
英文摘要Abstract Stars can be consumed (either tidally disrupted or swallowed whole) by massive black holes (MBHs) at galactic centers when they move into the vicinity of the MBHs. In this study, we investigate the rates of stellar consumption by central MBHs and their cosmic distributions, including the effects of triaxial galaxy shapes in enhancing the reservoir of low-angular-momentum stars and incorporating realistic galaxy distributions. We find that the enhancement in the stellar consumption rates due to triaxial galaxy shapes can be significant, by a factor of ~3 for MBH mass – and up to more than one order of magnitude for . Only for are the stellar consumption rates significantly higher in galaxies with steeper inner surface brightness profiles. The average (per galaxy) stellar consumption rates correlate with central MBH masses positively for and negatively for . The volumetric stellar tidal disruption rates are for MBHs in the mass range 105– at z?=?0; and the volumetric stellar consumption rates by MBHs with higher masses are , which can be the stellar tidal disruption rate if the high-mass BHs are extremely spinning Kerr BHs or the rate of being swallowed if those BHs are Schwarzschild ones. The volumetric stellar consumption rates decrease with increasing redshift, and the decrease is relatively mild for – and stronger for higher . Most of the stellar tidal disruption events (TDEs) at z?=?0 occur in galaxies with mass , and about 1%–2% of the TDEs can occur in high-mass galaxies with .
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-900-2-ABA950
源URL[http://ir.bao.ac.cn/handle/114a11/61870]  
专题中国科学院国家天文台
通讯作者Yu,Qingjuan
作者单位1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, People's Republic of China
2.Kavli Institute for Astronomy and Astrophysics, and School of Physics, Peking University, Beijing, 100871, People's Republic of China; yuqj@pku.edu.cn
3.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
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GB/T 7714
Chen,Yunfeng,Yu,Qingjuan,Lu,Youjun. Cosmic Distributions of Stellar Tidal Disruptions by Massive Black Holes at Galactic Centers[J]. The Astrophysical Journal,2020,900(2).
APA Chen,Yunfeng,Yu,Qingjuan,&Lu,Youjun.(2020).Cosmic Distributions of Stellar Tidal Disruptions by Massive Black Holes at Galactic Centers.The Astrophysical Journal,900(2).
MLA Chen,Yunfeng,et al."Cosmic Distributions of Stellar Tidal Disruptions by Massive Black Holes at Galactic Centers".The Astrophysical Journal 900.2(2020).

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来源:国家天文台

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