First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
Kazunori AkiyamaNational Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USAA. AlberdiInstituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, SpainW. AlefMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyKeiichi AsadaInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CRebecca AzulayObservatori Astronòmic, Universitat de València, C. Catedrático José Beltrán 2, E-46980 Paterna, València, SpainAnne-Kathrin BaczkoMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyDavid BallSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USAMislav BalokovićBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USAJ. BarrettMassachusetts Institute of Technology, Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USADan BintleyEast Asian Observatory, 660 N. A'ohoku Pl., Hilo, HI 96720, USALindy BlackburnCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAW. BolandNederlandse Onderzoekschool voor Astronomie (NOVA), PO Box 9513, 2300 RA Leiden, The NetherlandsKatherine L. BoumanCalifornia Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USAGeoffrey C. BowerMichael BremerInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceChristiaan D. BrinkerinkDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsRoger BrissendenBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USAS. BritzenMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyAvery E. BroderickWaterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1 CanadaDominique BroguièreInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceThomas BronzwaerDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsDo‐Young ByunKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaJ. E. CarlstromDepartment of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USAAndrew ChaelBlack Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USAChi‐kwan ChanSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USAShami ChatterjeeCornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USAKoushik ChatterjeeAnton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH, Amsterdam, The NetherlandsMing‐Tang ChenXiaopeng ChengIlje ChoUniversity of Science and Technology, Gajeong-ro 217, Yuseong-gu, Daejeon 34113, Republic of KoreaPierre ChristianCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAJ. E. ConwayDepartment of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, SwedenJ. M. CordesCornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USAG. CrewMassachusetts Institute of Technology, Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USAYuzhu CuiMizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, JapanJordy DavelaarDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsMariafelicia De LaurentisINFN Sez. di Napoli, Compl. Univ. di Monte S. Angelo, Edificio G, Via Cinthia, I-80126, Napoli, ItalyRoger DeaneCentre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Grahamstown 6140, South AfricaJessica DempseyEast Asian Observatory, 660 N. A'ohoku Pl., Hilo, HI 96720, USAG. DesvignesMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyJason DexterMax-Planck-Institut für Extraterrestrische Physik, Giessenbachstr. 1, D-85748 Garching, GermanySheperd S. DoelemanCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USARalph P. EatoughMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyH. FalckeDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsVincent L. FishMassachusetts Institute of Technology, Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USAEd FomalontNational Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USARaquel Fraga-EncinasDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsWilliam T. FreemanDepartment of Electrical Engineering and Computer Science, Massachusetts Institute of Technology, 32-D476, 77 Massachussetts Ave., Cambridge, MA 02142, USAPer FribergEast Asian Observatory, 660 N. A'ohoku Pl., Hilo, HI 96720, USAChristian M. FrommInstitut für Theoretische Physik, Goethe-Universität Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt am Main, GermanyJosé L. GómezInstituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, SpainPeter GalisonDepartment of History of Science, Harvard University, Cambridge, MA 02138, USACharles F. GammieDepartment of Physics, University of Illinois, 1110 West Green St, Urbana, IL 61801, USARoberto GarcíaInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceOlivier GentazInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceBoris GeorgievWaterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1 CanadaC. GoddiDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsRoman GoldInstitut für Theoretische Physik, Goethe-Universität Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt am Main, GermanyMinfeng GuMark GurwellCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAKazuhiro HadaMizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, JapanM. H. HechtMassachusetts Institute of Technology, Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USARonald HesperNOVA Sub-mm Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The NetherlandsLuis C. HoPaul T. P. HoInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CMareki HonmaMizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, JapanChih-Wei L. HuangInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CLei 磊 Huang 黄D. H. HughesInstituto Nacional de Astrofísica, Óptica y Electrónica. Apartado Postal 51 y 216, 72000. Puebla Pue., MéxicoShiro IkedaDepartment of Statistical Science, The Graduate University for Advanced Studies (SOKENDAI), 10-3 Midori-cho, Tachikawa, Tokyo 190-8562, JapanMakoto InoueInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CSara IssaounDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsD. J. JamesCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USABuell T. JannuziSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USAMichaël JanssenDepartment of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsBritton JeterDepartment of Physics and Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, ON, N2L 3G1, CanadaWu JiangMichael D. JohnsonCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USASvetlana G. JorstadAstronomical Institute, St. Petersburg University, Universitetskij pr., 28, Petrodvorets, 198504 St. Petersburg, RussiaTaehyun JungKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaMansour KaramiDepartment of Physics and Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, ON, N2L 3G1, CanadaR. KaruppusamyMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyTomohisa KawashimaNational Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JapanGarrett K. KeatingCenter for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USAMark KettenisJoint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The NetherlandsJae-Young KimMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyJunhan KimSteward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USAJongsoo KimKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaMotoki KinoKogakuin University of Technology & Engineering, Academic Support Center, 2665-1 Nakano, Hachioji, Tokyo 192-0015, JapanJun Yi KoayInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CPatrick M. KochInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CShoko KoyamaInstitute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.CMichael KramerMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyC. KrämerInstitut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406 Saint Martin d'Hères, FranceT. P. KrichbaumMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, GermanyC. Y. KuoPhysics Department, National Sun Yat-Sen University, No. 70, Lien-Hai Rd, Kaosiung City 80424, Taiwan, R.O.CTod R. LauerNational Optical Astronomy Observatory, 950 North Cherry Ave., Tucson, AZ 85719, USASang-Sung LeeKorea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of KoreaYanrong LiZhiyuan 志远 Li 李
2019en
ABI
Аннотация
Abstract When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon. To image and study this phenomenon, we have assembled the Event Horizon Telescope, a global very long baseline interferometry array observing at a wavelength of 1.3 mm. This allows us to reconstruct event-horizon-scale images of the supermassive black hole candidate in the center of the giant elliptical galaxy M87. We have resolved the central compact radio source as an asymmetric bright emission ring with a diameter of 42 ± 3 μ as, which is circular and encompasses a central depression in brightness with a flux ratio ≳10:1. The emission ring is recovered using different calibration and imaging schemes, with its diameter and width remaining stable over four different observations carried out in different days. Overall, the observed image is consistent with expectations for the shadow of a Kerr black hole as predicted by general relativity. The asymmetry in brightness in the ring can be explained in terms of relativistic beaming of the emission from a plasma rotating close to the speed of light around a black hole. We compare our images to an extensive library of ray-traced general-relativistic magnetohydrodynamic simulations of black holes and derive a central mass of M = (6.5 ± 0.7) × 10 9 M ⊙ . Our radio-wave observations thus provide powerful evidence for the presence of supermassive black holes in centers of galaxies and as the central engines of active galactic nuclei. They also present a new tool to explore gravity in its most extreme limit and on a mass scale that was so far not accessible.
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