First Sagittarius A* Event Horizon Telescope Results. V. Testing Astrophysical Models of the Galactic Center Black Hole

Author:

Event Horizon Telescope Collaboration ,Akiyama KazunoriORCID,Alberdi AntxonORCID,Alef Walter,Carlos Algaba JuanORCID,Anantua RichardORCID,Asada KeiichiORCID,Azulay RebeccaORCID,Bach UweORCID,Baczko Anne-KathrinORCID,Ball David,Baloković MislavORCID,Barrett JohnORCID,Bauböck MichiORCID,Benson Bradford A.ORCID,Bintley Dan,Blackburn LindyORCID,Blundell RaymondORCID,Bouman Katherine L.ORCID,Bower Geoffrey C.ORCID,Boyce HopeORCID,Bremer Michael,Brinkerink Christiaan D.ORCID,Brissenden RogerORCID,Britzen SilkeORCID,Broderick Avery E.ORCID,Broguiere DominiqueORCID,Bronzwaer ThomasORCID,Bustamante SandraORCID,Byun Do-YoungORCID,Carlstrom John E.ORCID,Ceccobello ChiaraORCID,Chael AndrewORCID,Chan Chi-kwanORCID,Chatterjee KoushikORCID,Chatterjee ShamiORCID,Chen Ming-TangORCID,Chen YongjunORCID,Cheng XiaopengORCID,Cho IljeORCID,Christian PierreORCID,Conroy Nicholas S.ORCID,Conway John E.ORCID,Cordes James M.ORCID,Crawford Thomas M.ORCID,Crew Geoffrey B.ORCID,Cruz-Osorio AlejandroORCID,Cui YuzhuORCID,Davelaar JordyORCID,De Laurentis MariafeliciaORCID,Deane RogerORCID,Dempsey JessicaORCID,Desvignes GregoryORCID,Dexter JasonORCID,Dhruv VedantORCID,Doeleman Sheperd S.ORCID,Dougal SeanORCID,Dzib Sergio A.ORCID,Eatough Ralph P.ORCID,Emami RaziehORCID,Falcke HeinoORCID,Farah JosephORCID,Fish Vincent L.ORCID,Fomalont EdORCID,Ford H. AlysonORCID,Fraga-Encinas RaquelORCID,Freeman William T.,Friberg PerORCID,Fromm Christian M.ORCID,Fuentes AntonioORCID,Galison PeterORCID,Gammie Charles F.ORCID,García RobertoORCID,Gentaz OlivierORCID,Georgiev BorisORCID,Goddi CiriacoORCID,Gold RomanORCID,Gómez-Ruiz Arturo I.ORCID,Gómez José L.ORCID,Gu MinfengORCID,Gurwell MarkORCID,Hada KazuhiroORCID,Haggard DarylORCID,Haworth Kari,Hecht Michael H.ORCID,Hesper RonaldORCID,Heumann DirkORCID,Ho Luis C.ORCID,Ho PaulORCID,Honma MarekiORCID,Huang Chih-Wei L.ORCID,Huang LeiORCID,Hughes David H.,Ikeda ShiroORCID,Violette Impellizzeri C. M.ORCID,Inoue MakotoORCID,Issaoun SaraORCID,James David J.ORCID,Jannuzi Buell T.ORCID,Janssen MichaelORCID,Jeter BrittonORCID,Jiang WuORCID,Jiménez-Rosales AlejandraORCID,Johnson Michael D.ORCID,Jorstad SvetlanaORCID,Joshi Abhishek V.ORCID,Jung TaehyunORCID,Karami MansourORCID,Karuppusamy RameshORCID,Kawashima TomohisaORCID,Keating Garrett K.ORCID,Kettenis MarkORCID,Kim Dong-JinORCID,Kim Jae-YoungORCID,Kim JongsooORCID,Kim JunhanORCID,Kino MotokiORCID,Koay Jun YiORCID,Kocherlakota PrashantORCID,Kofuji Yutaro,Koch Patrick M.ORCID,Koyama ShokoORCID,Kramer CarstenORCID,Kramer MichaelORCID,Krichbaum Thomas P.ORCID,Kuo Cheng-YuORCID,Bella Noemi LaORCID,Lauer Tod R.ORCID,Lee DaeyoungORCID,Lee Sang-SungORCID,Leung Po KinORCID,Levis AviadORCID,Li ZhiyuanORCID,Lico RoccoORCID,Lindahl GregORCID,Lindqvist MichaelORCID,Lisakov MikhailORCID,Liu JunORCID,Liu KuoORCID,Liuzzo ElisabettaORCID,Lo Wen-PingORCID,Lobanov Andrei P.ORCID,Loinard LaurentORCID,Lonsdale Colin J.ORCID,Lu Ru-SenORCID,Mao JirongORCID,Marchili NicolaORCID,Markoff SeraORCID,Marrone Daniel P.ORCID,Marscher Alan P.ORCID,Martí-Vidal IvánORCID,Matsushita SatokiORCID,Matthews Lynn D.ORCID,Medeiros LiaORCID,Menten Karl M.ORCID,Michalik DanielORCID,Mizuno IzumiORCID,Mizuno YosukeORCID,Moran James M.ORCID,Moriyama KotaroORCID,Moscibrodzka MonikaORCID,Müller CorneliaORCID,Mus AlejandroORCID,Musoke GibwaORCID,Myserlis IoannisORCID,Nadolski AndrewORCID,Nagai HiroshiORCID,Nagar Neil M.ORCID,Nakamura MasanoriORCID,Narayan RameshORCID,Narayanan GopalORCID,Natarajan IniyanORCID,Nathanail Antonios,Navarro Fuentes Santiago,Neilsen JoeyORCID,Neri RobertoORCID,Ni ChunchongORCID,Noutsos AristeidisORCID,Nowak Michael A.ORCID,Oh JunghwanORCID,Okino HirokiORCID,Olivares HéctorORCID,Ortiz-León Gisela N.ORCID,Oyama TomoakiORCID,Özel FeryalORCID,Palumbo Daniel C. M.ORCID,Filippos Paraschos GeorgiosORCID,Park JonghoORCID,Parsons HarrietORCID,Patel NimeshORCID,Pen Ue-LiORCID,Pesce Dominic W.ORCID,Piétu Vincent,Plambeck RichardORCID,PopStefanija Aleksandar,Porth OliverORCID,Pötzl Felix M.ORCID,Prather BenORCID,Preciado-López Jorge A.ORCID,Psaltis DimitriosORCID,Pu Hung-YiORCID,Ramakrishnan VenkatesshORCID,Rao RamprasadORCID,Rawlings Mark G.ORCID,Raymond Alexander W.ORCID,Rezzolla LucianoORCID,Ricarte AngeloORCID,Ripperda BartORCID,Roelofs FreekORCID,Rogers AlanORCID,Ros EduardoORCID,Romero-Cañizales CristinaORCID,Roshanineshat ArashORCID,Rottmann Helge,Roy Alan L.ORCID,Ruiz IgnacioORCID,Ruszczyk ChetORCID,Rygl Kazi L. J.ORCID,Sánchez SalvadorORCID,Sánchez-Argüelles DavidORCID,Sánchez-Portal MiguelORCID,Sasada MahitoORCID,Satapathy KaushikORCID,Savolainen TuomasORCID,Schloerb F. Peter,Schonfeld JonathanORCID,Schuster Karl-FriedrichORCID,Shao LijingORCID,Shen ZhiqiangORCID,Small DesORCID,Sohn Bong WonORCID,SooHoo JasonORCID,Souccar KamalORCID,Sun HeORCID,Tazaki FumieORCID,Tetarenko Alexandra J.ORCID,Tiede PaulORCID,Tilanus Remo P. J.ORCID,Titus MichaelORCID,Torne PabloORCID,Traianou EfthaliaORCID,Trent Tyler,Trippe SaschaORCID,Turk MatthewORCID,van Bemmel IlseORCID,van Langevelde Huib JanORCID,van Rossum Daniel R.ORCID,Vos JesseORCID,Wagner JanORCID,Ward-Thompson DerekORCID,Wardle JohnORCID,Weintroub JonathanORCID,Wex NorbertORCID,Wharton RobertORCID,Wielgus MaciekORCID,Wiik KajORCID,Witzel GuntherORCID,Wondrak Michael F.ORCID,Wong George N.ORCID,Wu QingwenORCID,Yamaguchi PaulORCID,Yoon DoosooORCID,Young AndréORCID,Young KenORCID,Younsi ZiriORCID,Yuan FengORCID,Yuan Ye-FeiORCID,Zensus J. AntonORCID,Zhang ShuoORCID,Zhao Guang-YaoORCID,Zhao Shan-ShanORCID,Chan Tin LokORCID,Qiu RichardORCID,Ressler SeanORCID,White ChrisORCID

Abstract

Abstract In this paper we provide a first physical interpretation for the Event Horizon Telescope's (EHT) 2017 observations of Sgr A*. Our main approach is to compare resolved EHT data at 230 GHz and unresolved non-EHT observations from radio to X-ray wavelengths to predictions from a library of models based on time-dependent general relativistic magnetohydrodynamics simulations, including aligned, tilted, and stellar-wind-fed simulations; radiative transfer is performed assuming both thermal and nonthermal electron distribution functions. We test the models against 11 constraints drawn from EHT 230 GHz data and observations at 86 GHz, 2.2 μm, and in the X-ray. All models fail at least one constraint. Light-curve variability provides a particularly severe constraint, failing nearly all strongly magnetized (magnetically arrested disk (MAD)) models and a large fraction of weakly magnetized models. A number of models fail only the variability constraints. We identify a promising cluster of these models, which are MAD and have inclination i ≤ 30°. They have accretion rate (5.2–9.5) × 10−9 M yr−1, bolometric luminosity (6.8–9.2) × 1035 erg s−1, and outflow power (1.3–4.8) × 1038 erg s−1. We also find that all models with i ≥ 70° fail at least two constraints, as do all models with equal ion and electron temperature; exploratory, nonthermal model sets tend to have higher 2.2 μm flux density; and the population of cold electrons is limited by X-ray constraints due to the risk of bremsstrahlung overproduction. Finally, we discuss physical and numerical limitations of the models, highlighting the possible importance of kinetic effects and duration of the simulations.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 311 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3