Scinovex
article Open AccessTop 1% cited

First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole

The Astrophysical Journal Letters · 2019 · Vol. 875(1) · pp. L6–L6
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 Garcı́aOlivier 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 YuanJ. A. ZensusGuang-Yao ZhaoShan-Shan ZhaoZiyan ZhuJoseph FarahZheng Meyer-ZhaoDaniel MichalikAndrew NadolskiHiroaki NishiokaNicolas PradelRurik A. PrimianiKamal SouccarLaura VertatschitschPaul Yamaguchi

Abstract

Abstract We present measurements of the properties of the central radio source in M87 using Event Horizon Telescope data obtained during the 2017 campaign. We develop and fit geometric crescent models (asymmetric rings with interior brightness depressions) using two independent sampling algorithms that consider distinct representations of the visibility data. We show that the crescent family of models is statistically preferred over other comparably complex geometric models that we explore. We calibrate the geometric model parameters using general relativistic magnetohydrodynamic (GRMHD) models of the emission region and estimate physical properties of the source. We further fit images generated from GRMHD models directly to the data. We compare the derived emission region and black hole parameters from these analyses with those recovered from reconstructed images. There is a remarkable consistency among all methods and data sets. We find that >50% of the total flux at arcsecond scales comes from near the horizon, and that the emission is dramatically suppressed interior to this region by a factor >10, providing direct evidence of the predicted shadow of a black hole. Across all methods, we measure a crescent diameter of 42 ± 3 μ as and constrain its fractional width to be <0.5. Associating the crescent feature with the emission surrounding the black hole shadow, we infer an angular gravitational radius of GM / Dc 2 = 3.8 ± 0.4 μ as. Folding in a distance measurement of gives a black hole mass of . This measurement from lensed emission near the event horizon is consistent with the presence of a central Kerr black hole, as predicted by the general theory of relativity.

Astrophysics and Cosmic PhenomenaAstrophysical Phenomena and ObservationsRadio Astronomy Observations and TechnologyPhysicsBlack hole (networking)Event horizonAstrophysicsAngular diameterRADIUSShadow (psychology)HorizonBrightnessEvent (particle physics)

Funding

  • National Science Foundation
  • Smithsonian Institution
  • U.S. Department of Energy
  • National Aeronautics and Space Administration
  • John Templeton Foundation
  • Gordon and Betty Moore Foundation
  • Harvard University
  • University of Chicago
  • 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
  • Government of Canada
  • Leverhulme Trust
  • 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
  • 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 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
  • 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
Citations
1,567
FWCI
316.38
field-weighted impact
References
131
Percentile
100%
vs. same field & year
Citations per year
Cited by
Hunting for extra dimensions in the shadow of M87*
Physical review. D/Physical review. D. · 2019 · 359 citations
Black hole shadows, photon rings, and lensing rings
Physical review. D/Physical review. D. · 2019 · 590 citations
First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
The Astrophysical Journal Letters · 2019 · 853 citations
First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
The Astrophysical Journal Letters · 2019 · 3,995 citations
First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
The Astrophysical Journal Letters · 2019 · 1,439 citations
References
<i>The Mathematical Theory of Black Holes</i>
Physics Today · 1984 · 2,183 citations
Electromagnetic extraction of energy from Kerr black holes
Monthly Notices of the Royal Astronomical Society · 1977 · 4,768 citations
Relativistic jets as compact radio sources
The Astrophysical Journal · 1979 · 1,934 citations
Hydromagnetic flows from accretion discs and the production of radio jets
Monthly Notices of the Royal Astronomical Society · 1982 · 3,830 citations
First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
The Astrophysical Journal Letters · 2019 · 1,439 citations
First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
The Astrophysical Journal Letters · 2019 · 1,394 citations
First M87 Event Horizon Telescope Results. II. Array and Instrumentation
The Astrophysical Journal Letters · 2019 · 1,045 citations
First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
The Astrophysical Journal Letters · 2019 · 853 citations
Citation Network

How this paper connects to the literature. Drag to explore, click any node to open that paper.