Probing jet base emission of M87* with the 2021 Event Horizon Telescope observations
Artikel i vetenskaplig tidskrift, 2026
We investigate the presence and spatial characteristics of the jet base emission in M87* at 230 GHz, enabled by the significantly enhanced (u,v) coverage in the 2021 Event Horizon Telescope (EHT) observations. The integration of the 12-m Kitt Peak Telescope (USA) and NOEMA (France) stations into the array introduces two critical intermediate-length baselines to SMT (USA) and IRAM 30-m (Spain), providing sensitivity to emission structures at spatial scales of ~250 μas and ~2500 μas (~0.02 pc and ~0.02 pc). Without these new baselines, previous EHT observations of the source in 2017 and 2018 lacked the capability to constrain emission on large scales, where a "missing flux"of order ~1 Jy is expected to reside. To probe these scales, we analyzed closure phases-robust against station-based gain calibration errors-and model the jet base emission using a simple Gaussian component offset from the compact ring emission at spatial separations > 100 μas. Our analysis revealed a Gaussian feature centered at (ΔRA ~ 320 μas, ΔDec. ~ 60 μ as), projected separation of ~5500 AU, with an estimated flux density of only ~60 mJy, implying that most of the missing flux identified in previous EHT studies had to originate from different, larger scales. Brighter emission at the relevant spatial scales is firmly ruled out, and the data do not favor more complex models. This component aligns with the inferred position of the large-scale jet and is therefore physically consistent with the emission of the jet base. While our findings point to detectable jet base emission at 230 GHz, the limited coverage provided by only two intermediate baselines limits our ability to robustly reconstruct its morphology. Consequently, we treated the recovered Gaussian as an upper limit on the jet base flux density. Future EHT observations with expanded intermediate baseline coverage will be essential to constrain the structure and nature of this component with higher precision.
Accretion, accretion disks
Gravitation
Relativistic processes
Black hole physics
Galaxies: individual: M 87*
Galaxies: jets
Författare
Saurabh
Max-Planck-Gesellschaft
Hendrik Müller
National Radio Astronomy Observatory
S. von Fellenberg
Max-Planck-Gesellschaft
Institut canadien d'astrophysique théorique
Paul Tiede
Harvard University
Harvard-Smithsonian Center for Astrophysics
Michael Janssen
Radboud Universiteit
Max-Planck-Gesellschaft
Lindy Blackburn
Harvard-Smithsonian Center for Astrophysics
Harvard University
Avery E. Broderick
Perimeter Institute for Theoretical Physics
University of Waterloo
Erandi Chavez
Harvard-Smithsonian Center for Astrophysics
Boris Georgiev
University of Arizona
T.P. Krichbaum
Max-Planck-Gesellschaft
Kotaro Moriyama
Johann Wolfgang Goethe Universität Frankfurt am Main
National Astronomical Observatory of Japan
Dhanya G. Nair
Max-Planck-Gesellschaft
Iniyan Natarajan
Harvard University
Harvard-Smithsonian Center for Astrophysics
Jongho Park
Academia Sinica
Kyung Hee University
Andrew Thomas West
University of Arizona
M. Wielgus
Consejo Superior de Investigaciones Científicas (CSIC)
Kazunori Akiyama
Harvard University
Massachusetts Institute of Technology (MIT)
National Astronomical Observatory of Japan
E. Albentosa-Ruiz
Universitat de Valencia
Antxon Alberdi
Consejo Superior de Investigaciones Científicas (CSIC)
Walter Alef
Max-Planck-Gesellschaft
Juan-Carlos Algaba
University of Malaya
Richard Anantua
Rice University
Harvard-Smithsonian Center for Astrophysics
University of Texas
Harvard University
K. Asada
Kyung Hee University
R. Azulay
Universitat de Valencia
Max-Planck-Gesellschaft
U. Bach
Max-Planck-Gesellschaft
Anne-Kathrin Baczko
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
David Ball
University of Arizona
Mislav Baloković
Yale University
Bidisha Bandyopadhyay
Universidad de Concepción
John Barrett
Massachusetts Institute of Technology (MIT)
M. Bauböck
University of Illinois
Bradford A. Benson
Fermi National Accelerator Laboratory
University of Chicago
Dan Bintley
East Asian Observatory
James Clerk Maxwell Telescope
R. Blundell
Harvard-Smithsonian Center for Astrophysics
K. L. Bouman
California Institute of Technology (Caltech)
G. C. Bower
Academia Sinica
James Clerk Maxwell Telescope
East Asian Observatory
M. Bremer
Institut de Radioastronomie Millimétrique (IRAM)
Roger Brissenden
Harvard-Smithsonian Center for Astrophysics
Silke Britzen
Max-Planck-Gesellschaft
D. Broguière
Institut de Radioastronomie Millimétrique (IRAM)
Thomas Bronzwaer
Radboud Universiteit
Sandra Bustamente
University of Massachusetts
Douglas Ferreira Carlos
Universidade de Sao Paulo (USP)
J. E. Carlstrom
University of Chicago
A. Chael
Princeton University
Chi Kwan Chan
University of Arizona
Dominic O. Chang
Harvard-Smithsonian Center for Astrophysics
Harvard University
Koushik Chatterjee
Harvard-Smithsonian Center for Astrophysics
University of Maryland
Harvard University
S. Chatterjee
Cornell University
Ming Tang Chen
Academia Sinica
Yongjun Chen
Chinese Academy of Sciences
X. P. Cheng
Korea Astronomy and Space Science Institute
Paul Chichura
University of Chicago
I. Cho
Academia Sinica
Yonsei University
Korea Astronomy and Space Science Institute
Pierre Christian
WattTime
Nicholas S. Conroy
University of Illinois
Harvard-Smithsonian Center for Astrophysics
John Conway
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
Thomas M. Crawford
University of Chicago
G. Crew
Consejo Superior de Investigaciones Científicas (CSIC)
Alejandro Cruz-Osorio
Johann Wolfgang Goethe Universität Frankfurt am Main
Universidad Nacional Autónoma de México
Yuzhu Cui
Central China Normal University
Brandon Curd
Harvard University
Harvard-Smithsonian Center for Astrophysics
University of Malaya
Rohan Dahale
Academia Sinica
Jordy Davelaar
Princeton University
Mariafelicia De Laurentis
Universita degli Studi di Napoli Federico II
Istituto Nazionale di Fisica Nucleare
R. P. Deane
Universiteit van Pretoria
University of Witwatersrand
Rhodes University
Gregory Desvignes
Centre national de la recherche scientifique (CNRS)
Max-Planck-Gesellschaft
Jason Dexter
University of Colorado
Vedant Dhruv
University of Illinois
Indu K. Dihingia
Shanghai Jiao Tong University
S. Doeleman
Harvard-Smithsonian Center for Astrophysics
Harvard University
Sergio A. Dzib
Max-Planck-Gesellschaft
Ralph P. Eatough
Max-Planck-Gesellschaft
Chinese Academy of Sciences
Razieh Emami
Harvard-Smithsonian Center for Astrophysics
H.D. Falcke
Radboud Universiteit
Joseph R. Farah
Las Cumbres Observatory Global Telescope Network
University of California
V. Fish
Consejo Superior de Investigaciones Científicas (CSIC)
E. Fomalont
National Radio Astronomy Observatory
Marianna Foschi
Academia Sinica
R. Fraga-Encinas
Radboud Universiteit
William T. Freeman
Google Inc.
Massachusetts Institute of Technology (MIT)
P. Friberg
James Clerk Maxwell Telescope
East Asian Observatory
Christian M. Fromm
Johann Wolfgang Goethe Universität Frankfurt am Main
Max-Planck-Gesellschaft
Julius-Maximilians Universität Würzburg
Antonio Fuentes
Academia Sinica
Peter Galison
Harvard University
Charles F. Gammie
University of Illinois
Roberto Garcia
Institut de Radioastronomie Millimétrique (IRAM)
Olivier Gentaz
Institut de Radioastronomie Millimétrique (IRAM)
C. Goddi
Universita degli Studi di Cagliari
Universidade de Sao Paulo (USP)
Istituto Nazionale di Fisica Nucleare
R. Gold
Universität Heidelberg
Syddansk Universitet
Arturo I. Gómez-Ruiz
Instituto Nacional de Astrofísica, Óptica y Electrońica
J. L. Gomez
Academia Sinica
Minfeng Gu
Chinese Academy of Sciences
M. Gurwell
Harvard-Smithsonian Center for Astrophysics
K. Hada
National Astronomical Observatory of Japan
Nagoya University
Daryl Haggard
McGill University
R. Hesper
Rijksuniversiteit Groningen
Dirk Heumann
University of Arizona
Luis C. Ho
Peking University
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 706 A27Ämneskategorier (SSIF 2025)
Fusion, plasma och rymdfysik
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202557022