中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Ring Asymmetry and Spin in M87

文献类型:期刊论文

作者Bernshteyn, Vadim2,3; Conroy, Nicholas S.4; Baubock, Michi2; Tiede, Paul5,6; Joshi, Abhishek V.2,7; Prather, Ben S.2,8; Gammie, Charles F.2,4,7,9; Akiyama, Kazunori6,10,11; Albentosa-Ruiz, Ezequiel12; Alberdi, Antxon13
刊名ASTROPHYSICAL JOURNAL
出版日期2026-04-01
卷号1000期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ae34af
产权排序第112完成单位
文献子类Article
英文摘要Event Horizon Telescope (EHT) images of the supermassive black hole M87* depict an asymmetric ring of emission. General relativistic magnetohydrodynamic (GRMHD) models of M87* and its accretion disk predict that the amplitude and location of the ring's peak brightness asymmetry should fluctuate due to turbulence in the source plasma. We compare the observed distribution of brightness asymmetry amplitudes to the simulated distribution in GRMHD models, across varying black hole spin a(*). We show that, for strongly magnetized (MAD) models, three epochs of EHT data marginally disfavor divided by a(*)divided by less than or similar to 0.2. This is consistent with the Blandford-Znajek model for M87's jet, which predicts that M87* should have nonzero spin. We show quantitatively how future observations could improve spin constraints and discuss how improved spin constraints could distinguish between differing jet-launching mechanisms and black hole growth scenarios.
学科主题天文学 ; 星系与宇宙学
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词ADVECTION-DOMINATED ACCRETION ; SUPERMASSIVE BLACK-HOLE ; SAGITTARIUS-A-ASTERISK ; MAGNETICALLY ARRESTED ACCRETION ; EVENT HORIZON ; MAGNETOHYDRODYNAMIC SIMULATIONS ; GALACTIC-CENTER ; X-RAY ; MODELS ; DISKS
资助项目NASA divided by Science Mission Directorate (SMD)[80NSSC24K1475]; National Science Foundation (NSF)[AST 17-16327]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001723355600001
出版者IOP Publishing Ltd
资助机构NASA divided by Science Mission Directorate (SMD)[80NSSC24K1475] ; National Science Foundation (NSF)[AST 17-16327]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/29133]  
专题云南天文台_中国科学院天体结构与演化重点实验室
通讯作者Conroy, Nicholas S.
作者单位1.East Asian Observatory, 660 N. A’ohoku Place, Hilo, HI 96720, USA;
2.Department of Physics, University of Illinois, 1110 West Green Street, Urbana, IL 61801, USA;
3.Steward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA;
4.Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801, USA; nconroy2@illinois.edu;
5.Center for Astrophysics ∣Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA;
6.Black Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USA;
7.Illinois Center for Advanced Study of the Universe, 1110 West Green Street, Urbana, IL 61801, USA;
8.Los Alamos National Lab, Los Alamos, NM, 87545, USA;
9.National Center for Supercomputing Applications, 605 East Springfield Avenue, Champaign, IL 61820, USA;
10.Massachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USA;
推荐引用方式
GB/T 7714
Bernshteyn, Vadim,Conroy, Nicholas S.,Baubock, Michi,et al. Ring Asymmetry and Spin in M87[J]. ASTROPHYSICAL JOURNAL,2026,1000(2).
APA Bernshteyn, Vadim.,Conroy, Nicholas S..,Baubock, Michi.,Tiede, Paul.,Joshi, Abhishek V..,...&Zhao, Guang-Yao.(2026).Ring Asymmetry and Spin in M87.ASTROPHYSICAL JOURNAL,1000(2).
MLA Bernshteyn, Vadim,et al."Ring Asymmetry and Spin in M87".ASTROPHYSICAL JOURNAL 1000.2(2026).

入库方式: OAI收割

来源:云南天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。