The Photon Ring in M87*
Artikel i vetenskaplig tidskrift, 2022

We report measurements of the gravitationally lensed secondary image—the first in an infinite series of so-called “photon rings”—around the supermassive black hole M87* via simultaneous modeling and imaging of the 2017 Event Horizon Telescope (EHT) observations. The inferred ring size remains constant across the seven days of the 2017 EHT observing campaign and is consistent with theoretical expectations, providing clear evidence that such measurements probe spacetime and a striking confirmation of the models underlying the first set of EHT results. The residual diffuse emission evolves on timescales comparable to one week. We are able to detect with high significance a southwestern extension consistent with that expected from the base of a jet that is rapidly rotating in the clockwise direction. This result adds further support to the identification of the jet in M87* with a black hole spin-driven outflow, launched via the Blandford-Znajek process. We present three revised estimates for the mass of M87* based on identifying the modeled thin ring component with the bright ringlike features seen in simulated images, one of which is only weakly sensitive to the astrophysics of the emission region. All three estimates agree with each other and previously reported values. Our strongest mass constraint combines information from both the ring and the diffuse emission region, which together imply a mass-to-distance ratio of 4.20 − 0.06 + 0.12 μ as and a corresponding black hole mass of (7.13 ± 0.39) × 109 M ⊙, where the error on the latter is now dominated by the systematic uncertainty arising from the uncertain distance to M87*.

Författare

Avery E. Broderick

University of Waterloo

Perimeter Institute for Theoretical Physics

Dominic W. Pesce

Harvard-Smithsonian Center for Astrophysics

Harvard University

R. Gold

Syddansk Universitet

Paul Tiede

Harvard University

University of Waterloo

Perimeter Institute for Theoretical Physics

Harvard-Smithsonian Center for Astrophysics

Hung-Yi Pu

National Taiwan Normal University

Academia Sinica

National Center for Theoretical Sciences Taiwan

Richard Anantua

Harvard-Smithsonian Center for Astrophysics

Harvard University

The University of Texas at San Antonio

Silke Britzen

Max-Planck-Gesellschaft

Chiara Ceccobello

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Koushik Chatterjee

Harvard University

Harvard-Smithsonian Center for Astrophysics

Yongjun Chen

Shanghai Astronomical Observatory

Chinese Academy of Sciences

Nicholas S. Conroy

University of Illinois

Harvard-Smithsonian Center for Astrophysics

G. Crew

Massachusetts Institute of Technology (MIT)

Alejandro Cruz-Osorio

Johann Wolfgang Goethe Universität Frankfurt am Main

Yuzhu Cui

National Astronomical Observatory of Japan

The Graduate University for Advanced Studies (SOKENDAI)

Shanghai Jiao Tong University

S. Doeleman

Harvard-Smithsonian Center for Astrophysics

Harvard University

Razieh Emami

Harvard-Smithsonian Center for Astrophysics

Joseph R. Farah

Las Cumbres Observatory Global Telescope Network

University of California

Christian M. Fromm

Julius-Maximilians Universität Würzburg

Max-Planck-Gesellschaft

Johann Wolfgang Goethe Universität Frankfurt am Main

Peter Galison

Harvard University

Boris Georgiev

University of Waterloo

Perimeter Institute for Theoretical Physics

Luis C. Ho

Beijing University of Technology

David J. James

ASTRAVEO

Britton Jeter

Academia Sinica

Alejandra Jimenez-Rosales

Radboud Universiteit

Jun Yi Koay

Academia Sinica

C. Kramer

Institut de Radioastronomie Millimétrique (IRAM)

T.P. Krichbaum

Max-Planck-Gesellschaft

Sang Sung Lee

Korea Astronomy and Space Science Institute

University of Science and Technology (UST)

Michael Lindqvist

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

Ivan Marti-Vidal

Universitat de Valencia

K. Menten

Max-Planck-Gesellschaft

Yosuke Mizuno

Shanghai Jiao Tong University

Johann Wolfgang Goethe Universität Frankfurt am Main

James M. Moran

Harvard-Smithsonian Center for Astrophysics

Harvard University

M. Mościbrodzka

Radboud Universiteit

Antonios Nathanail

Johann Wolfgang Goethe Universität Frankfurt am Main

Joseph Neilsen

Villanova University

Chunchong Ni

University of Waterloo

Perimeter Institute for Theoretical Physics

Jongho Park

Academia Sinica

Vincent Piétu

Institut de Radioastronomie Millimétrique (IRAM)

Luciano Rezzolla

Johann Wolfgang Goethe Universität Frankfurt am Main

Angelo Ricarte

Harvard-Smithsonian Center for Astrophysics

Harvard University

Bart Ripperda

Princeton University

Flatiron Institute

Lijing Shao

Max-Planck-Gesellschaft

Beijing University of Technology

Fumie Tazaki

National Astronomical Observatory of Japan

Kenji Toma

Tohoku University

Pablo Torne

Max-Planck-Gesellschaft

J. Weintroub

Harvard-Smithsonian Center for Astrophysics

Harvard University

M. Wielgus

Max-Planck-Gesellschaft

Feng Yuan

Shanghai Astronomical Observatory

Shan-Shan Zhao

Shanghai Astronomical Observatory

Shuo Zhang

Bard College

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 935 1 61

Ämneskategorier

Subatomär fysik

Astronomi, astrofysik och kosmologi

Datorseende och robotik (autonoma system)

DOI

10.3847/1538-4357/ac7c1d

Mer information

Senast uppdaterat

2022-10-07