First M87 Event Horizon Telescope Results. I. the Shadow of the Supermassive Black Hole
Artikel i vetenskaplig tidskrift, 2019
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 μas, 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 o . 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.
Författare
Kazunori Akiyama
Harvard University
Massachusetts Institute of Technology (MIT)
National Astronomical Observatory of Japan
National Radio Astronomy Observatory
Antxon Alberdi
Consejo Superior de Investigaciones Científicas (CSIC)
Walter Alef
Max-Planck-Gesellschaft
K. Asada
Academia Sinica
R. Azulay
Universitat de Valencia
Max-Planck-Gesellschaft
A. K. Baczko
Max-Planck-Gesellschaft
David Ball
University of Arizona
Mislav Baloković
Harvard-Smithsonian Center for Astrophysics
Harvard University
John Barrett
Massachusetts Institute of Technology (MIT)
Dan Bintley
East Asian Observatory
Lindy Blackburn
Harvard-Smithsonian Center for Astrophysics
Harvard University
W. Boland
Nederlandse Onderzoekschool voor Astronomie (NOVA)
K. L. Bouman
Harvard-Smithsonian Center for Astrophysics
Harvard University
California Institute of Technology (Caltech)
G. C. Bower
Academia Sinica
M. Bremer
Institut de Radioastronomie Millimétrique (IRAM)
C. D. Brinkerink
Radboud Universiteit
Roger Brissenden
Harvard-Smithsonian Center for Astrophysics
Harvard University
Silke Britzen
Max-Planck-Gesellschaft
Avery E. Broderick
University of Waterloo
Perimeter Institute for Theoretical Physics
D. Broguière
Institut de Radioastronomie Millimétrique (IRAM)
Thomas Bronzwaer
Radboud Universiteit
Do Young Byun
Korea Astronomy and Space Science Institute
University of Science and Technology (UST)
J. E. Carlstrom
University of Chicago
A. Chael
Harvard University
Harvard-Smithsonian Center for Astrophysics
Chi Kwan Chan
University of Arizona
S. Chatterjee
Cornell University
Koushik Chatterjee
Universiteit Van Amsterdam
Ming Tang Chen
Academia Sinica
Yongjun Chen
Chinese Academy of Sciences
I. Cho
University of Science and Technology (UST)
Korea Astronomy and Space Science Institute
Pierre Christian
Harvard-Smithsonian Center for Astrophysics
University of Arizona
John Conway
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
James M. Cordes
Cornell University
G. Crew
Massachusetts Institute of Technology (MIT)
Yuzhu Cui
The Graduate University for Advanced Studies (SOKENDAI)
National Astronomical Observatory of Japan
Jordy Davelaar
Radboud Universiteit
Mariafelicia De Laurentis
Universita degli Studi di Napoli Federico II
Johann Wolfgang Goethe Universität Frankfurt am Main
R. P. Deane
Universiteit van Pretoria
Rhodes University
Jessica Dempsey
East Asian Observatory
Gregory Desvignes
Max-Planck-Gesellschaft
Jason Dexter
Max-Planck-Gesellschaft
S. Doeleman
Harvard-Smithsonian Center for Astrophysics
Harvard University
Ralph P. Eatough
Max-Planck-Gesellschaft
H.D. Falcke
Radboud Universiteit
V. Fish
Massachusetts Institute of Technology (MIT)
E. Fomalont
National Radio Astronomy Observatory
R. Fraga-Encinas
Radboud Universiteit
William T. Freeman
Massachusetts Institute of Technology (MIT)
Google Inc.
P. Friberg
East Asian Observatory
Christian M. Fromm
Johann Wolfgang Goethe Universität Frankfurt am Main
J. L. Gomez
Consejo Superior de Investigaciones Científicas (CSIC)
Peter Galison
Harvard University
Charles F. Gammie
University of Illinois
Roberto Garcia
Institut de Radioastronomie Millimétrique (IRAM)
Olivier Gentaz
Institut de Radioastronomie Millimétrique (IRAM)
Boris Georgiev
University of Waterloo
C. Goddi
Radboud Universiteit
Universiteit Leiden
R. Gold
Johann Wolfgang Goethe Universität Frankfurt am Main
Minfeng Gu
Chinese Academy of Sciences
M. Gurwell
Harvard-Smithsonian Center for Astrophysics
K. Hada
National Astronomical Observatory of Japan
The Graduate University for Advanced Studies (SOKENDAI)
Michael H. Hecht
Massachusetts Institute of Technology (MIT)
R. Hesper
Rijksuniversiteit Groningen
Luis C. Ho
Beijing University of Technology
Paul Ho
Academia Sinica
Mareki Honma
National Astronomical Observatory of Japan
The Graduate University for Advanced Studies (SOKENDAI)
Chih Wei L. Huang
Academia Sinica
Lei Huang
Chinese Academy of Sciences
D. Hughes
Instituto Nacional de Astrofísica, Óptica y Electrońica
Shiro Ikeda
University of Tokyo
The Graduate University for Advanced Studies (SOKENDAI)
The Institute of Statistical Mathematics
National Astronomical Observatory of Japan
Makoto Inoue
Academia Sinica
S. Issaoun
Radboud Universiteit
David J. James
Harvard-Smithsonian Center for Astrophysics
Harvard University
Buell T. Jannuzi
University of Arizona
M. Janßen
Radboud Universiteit
Britton Jeter
University of Waterloo
Wu Jiang
Chinese Academy of Sciences
Michael D. Johnson
Harvard-Smithsonian Center for Astrophysics
Harvard University
S.G. Jorstad
Boston University
Saint Petersburg State University - Spsu
Taehyun Jung
University of Science and Technology (UST)
Korea Astronomy and Space Science Institute
Mansour Karami
University of Waterloo
Perimeter Institute for Theoretical Physics
R. Karuppusamy
Max-Planck-Gesellschaft
Tomohisa Kawashima
National Astronomical Observatory of Japan
G. Keating
Harvard-Smithsonian Center for Astrophysics
M. M. Kettenis
Joint Institute for VLBI in Europe (JIVE)
Jae Young Kim
Max-Planck-Gesellschaft
Junhan Kim
University of Arizona
Jongsoo Kim
Korea Astronomy and Space Science Institute
M. Kino
Kogakuin University of Technology and Engineering
National Astronomical Observatory of Japan
Jun Yi Koay
Academia Sinica
Patrick M. Koch
Academia Sinica
Shoko Koyama
Academia Sinica
M. Kramer
Max-Planck-Gesellschaft
C. Kramer
Institut de Radioastronomie Millimétrique (IRAM)
T.P. Krichbaum
Max-Planck-Gesellschaft
Cheng Yu Kuo
National Sun Yat-Sen University
Tod R. Lauer
National Optical Astronomy Observatory
Sang Sung Lee
Korea Astronomy and Space Science Institute
Yan Rong Li
Chinese Academy of Sciences
Astrophysical Journal Letters
2041-8205 (ISSN) 2041-8213 (eISSN)
Vol. 875 1 L1Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.3847/2041-8213/ab0ec7