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First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring

The Astrophysical Journal Letters · 2019 · Vol. 875(1) · pp. L5–L5
Kazunori AkiyamaA. AlberdiW. AlefKeiichi AsadaRebecca AzulayAnne-Kathrin BaczkoDavid BallMislav BalokovićJohn BarrettDan BintleyLindy BlackburnW. BolandKatherine L. BoumanGeoffrey C. BowerMichael BremerChristiaan D. BrinkerinkRoger BrissendenS. BritzenAvery E. BroderickDominique BroguièreThomas BronzwaerDo‐Young ByunJ. E. CarlstromAndrew ChaelChi‐kwan ChanShami ChatterjeeKoushik ChatterjeeMing‐Tang ChenXiaopeng ChengIlje ChoPierre ChristianJ. E. ConwayJ. M. CordesG. CrewYuzhu CuiJordy DavelaarMariafelicia De LaurentisRoger DeaneJessica DempseyG. DesvignesJason DexterSheperd S. DoelemanRalph P. EatoughH. FalckeVincent L. FishEd FomalontRaquel Fraga-EncinasPer FribergChristian M. FrommJosé L. GómezPeter GalisonCharles F. GammieRoberto GarcíaOlivier GentazBoris GeorgievC. GoddiRoman GoldMinfeng GuMark GurwellKazuhiro HadaM. H. HechtRonald HesperLuis C. HoPaul T. P. HoMareki HonmaChih-Wei L. HuangLei 磊 Huang 黄D. H. HughesShiro IkedaMakoto InoueSara IssaounD. J. JamesBuell T. JannuziMichaël JanssenBritton JeterWu JiangMichael D. JohnsonSvetlana G. JorstadTaehyun JungMansour KaramiR. KaruppusamyTomohisa KawashimaGarrett K. KeatingMark KettenisJae-Young KimJunhan KimJongsoo KimMotoki KinoJun Yi KoayPatrick M. KochShoko KoyamaM. KrämerC. KrämerT. P. KrichbaumCheng‐Yu KuoTod R. LauerSang-Sung LeeYan-Rong LiZhiyuan 志远 Li 李M. LindqvistKuo LiuElisabetta LiuzzoWen-Ping LoA. P. LobanovLaurent LoinardC. J. LonsdaleRu-Sen LuNicholas R. MacDonaldJirong 基荣 Mao 毛Sera MarkoffDaniel P. MarroneAlan P. MarscherI. Martí‐VidalSatoki MatsushitaLynn D. MatthewsLia MedeirosK. M. MentenYosuke MizunoIzumi MizunoJ. M. MoranKotaro MoriyamaMonika MościbrodzkaCornelia MüllerHiroshi NagaiNeil M. NagarMasanori NakamuraRamesh NarayanGopal NarayananIniyan NatarajanR. NeriChunchong NiA. NoutsosHiroki OkinoHéctor OlivaresTomoaki OyamaFeryal ÖzelDaniel C. M. PalumboNimesh PatelUe‐Li PenDominic W. PesceVincent PiétuR. L. PlambeckAleksandar PopStefanijaOliver PorthBen PratherJorge A. Preciado-LópezDimitrios PsaltisHung-Yi PuVenkatessh RamakrishnanRamprasad RaoMark G. RawlingsAlexander W. RaymondLuciano RezzollaBart RipperdaFreek RoelofsA. E. E. RogersE. RosMel RoseArash RoshanineshatHelge RottmannA. L. RoyChet RuszczykBenjamin R. RyanK. L. J. RyglSalvador SánchezDavid Sánchez-ArgüellesMahito SasadaT. SavolainenF. Peter SchloerbK. SchüsterLijing ShaoZhi-Qiang ShenDes SmallBong Won SohnJason SoohooFumie TazakiPaul TiedeR. P. J. TilanusMichael S. TitusKenji TomaPablo TornéTyler TrentSascha TrippeShuichiro TsudaIlse van BemmelHuib Jan van LangeveldeDaniel R. van RossumJan WagnerJ. F. C. WardleJonathan WeintroubNorbert WexRobert WhartonMaciek WielgusGeorge N. WongQingwen 庆文 Wu 吴André YoungKen YoungZiri YounsiFeng 峰 Yuan 袁Ye-Fei 业飞 Yuan 袁J. A. ZensusGuang-Yao ZhaoShan-Shan ZhaoZiyan ZhuJ. AnczarskiFrederick K. BaganoffA. EckartJoseph FarahDaryl HaggardZheng Meyer-ZhaoDaniel MichalikAndrew NadolskiJoey NeilsenHiroaki NishiokaMichael A. NowakNicolas PradelRurik A. PrimianiKamal SouccarLaura VertatschitschPaul YamaguchiShuo Zhang

Abstract

Abstract The Event Horizon Telescope (EHT) has mapped the central compact radio source of the elliptical galaxy M87 at 1.3 mm with unprecedented angular resolution. Here we consider the physical implications of the asymmetric ring seen in the 2017 EHT data. To this end, we construct a large library of models based on general relativistic magnetohydrodynamic (GRMHD) simulations and synthetic images produced by general relativistic ray tracing. We compare the observed visibilities with this library and confirm that the asymmetric ring is consistent with earlier predictions of strong gravitational lensing of synchrotron emission from a hot plasma orbiting near the black hole event horizon. The ring radius and ring asymmetry depend on black hole mass and spin, respectively, and both are therefore expected to be stable when observed in future EHT campaigns. Overall, the observed image is consistent with expectations for the shadow of a spinning Kerr black hole as predicted by general relativity. If the black hole spin and M87’s large scale jet are aligned, then the black hole spin vector is pointed away from Earth. Models in our library of non-spinning black holes are inconsistent with the observations as they do not produce sufficiently powerful jets. At the same time, in those models that produce a sufficiently powerful jet, the latter is powered by extraction of black hole spin energy through mechanisms akin to the Blandford-Znajek process. We briefly consider alternatives to a black hole for the central compact object. Analysis of existing EHT polarization data and data taken simultaneously at other wavelengths will soon enable new tests of the GRMHD models, as will future EHT campaigns at 230 and 345 GHz.

Pulsars and Gravitational Waves ResearchAstrophysical Phenomena and ObservationsAstrophysics and Cosmic PhenomenaPhysicsEvent horizonBlack hole (networking)Supermassive black holeAstrophysicsSchwarzschild radiusKerr metricRotating black holeBinary black holeSpin-flip

Funding

  • National Science Foundation
  • Smithsonian Institution
  • U.S. Department of Energy
  • National Aeronautics and Space Administration
  • John Templeton Foundation
  • Gordon and Betty Moore Foundation
  • Kavli Foundation
  • Harvard University
  • University of Chicago
  • Canadian Institute for Advanced Research
  • University of Arizona
  • Innovation, Science and Economic Development Canada
  • Compute Canada
  • Ministerio de Ciencia, Innovación y Universidades
  • National Radio Astronomy Observatory
  • Associated Universities
  • International Max Planck Research School for Environmental, Cellular and Molecular Microbiology
  • Joint Institute for Computational Fundamental Science
  • Government of Canada
  • Leverhulme Trust
  • European Commission
  • National Research Foundation
  • Department of Science and Technology, Ministry of Science and Technology, India
  • Ministry of Education, Culture, Sports, Science and Technology
  • National Natural Science Foundation of China
  • Academia Sinica
  • Academy of Finland
  • Chinese Academy of Sciences
  • Consejo Nacional de Ciencia y Tecnología
  • Nederlandse Organisatie voor Wetenschappelijk Onderzoek
  • Ministerio de Economía y Competitividad
  • Generalitat Valenciana
  • Nuclear Safety and Security Commission
  • Korea Astronomy and Space Science Institute
  • National Research Foundation of Korea
  • Max-Planck-Gesellschaft
  • Vetenskapsrådet
  • China Scholarship Council
  • European Southern Observatory
  • Centre National de la Recherche Scientifique
  • Universidad Nacional Autónoma de México
  • National Astronomical Observatory of Japan
  • Russian Science Foundation
  • Ministero dello Sviluppo Economico
  • Recruitment Program of Global Experts
  • Istituto Nazionale di Fisica Nucleare
  • Instituto Nacional de Astrofísica, Óptica y Electrónica
  • Instituto de Astrofísica de Andalucía
  • Institut Périmètre de physique théorique
  • Toray Science Foundation
  • National Nuclear Security Administration
  • Natural Sciences and Engineering Research Council of Canada
  • Japan Society for the Promotion of Science
  • Comisión Nacional de Investigación Científica y Tecnológica
  • Fonds de recherche du Québec – Nature et technologies
  • Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México
  • National Institutes of Natural Sciences
  • National Key Research and Development Program of China
  • Office of International Science and Engineering
  • Los Alamos National Laboratory
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