Ordered magnetic fields around the 3C 84 central black hole
Artikel i vetenskaplig tidskrift, 2024
Context. 3C 84 is a nearby radio source with a complex total intensity structure, showing linear polarisation and spectral patterns. A detailed investigation of the central engine region necessitates the use of very-long-baseline interferometry (VLBI) above the hitherto available maximum frequency of 86 GHz. Aims. Using ultrahigh resolution VLBI observations at the currently highest available frequency of 228 GHz, we aim to perform a direct detection of compact structures and understand the physical conditions in the compact region of 3C 84.
Methods. We used Event Horizon Telescope (EHT) 228 GHz observations and, given the limited (u, v)-coverage, applied geometric model fitting to the data. Furthermore, we employed quasi-simultaneously observed, ancillary multi-frequency VLBI data for the source in order to carry out a comprehensive analysis of the core structure.
Results. We report the detection of a highly ordered, strong magnetic field around the central, supermassive black hole of 3C 84. The brightness temperature analysis suggests that the system is in equipartition. We also determined a turnover frequency of νm = (113 ± 4) GHz, a corresponding synchrotron self-absorbed magnetic field of BSSA = (2.9 ± 1.6) G, and an equipartition magnetic field of Beq = (5.2 ± 0.6) G. Three components are resolved with the highest fractional polarisation detected for this object (mnet = (17.0 ± 3.9)%). The positions of the components are compatible with those seen in low-frequency VLBI observations since 2017-2018. We report a steeply negative slope of the spectrum at 228 GHz. We used these findings to test existing models of jet formation, propagation, and Faraday rotation in 3C 84.
Conclusions. The findings of our investigation into different flow geometries and black hole spins support an advection-dominated accretion flow in a magnetically arrested state around a rapidly rotating supermassive black hole as a model of the jet-launching system in the core of 3C 84. However, systematic uncertainties due to the limited (u, v)-coverage, however, cannot be ignored. Our upcoming work using new EHT data, which offer full imaging capabilities, will shed more light on the compact region of 3C 84.
Methods. We used Event Horizon Telescope (EHT) 228 GHz observations and, given the limited (u, v)-coverage, applied geometric model fitting to the data. Furthermore, we employed quasi-simultaneously observed, ancillary multi-frequency VLBI data for the source in order to carry out a comprehensive analysis of the core structure.
Results. We report the detection of a highly ordered, strong magnetic field around the central, supermassive black hole of 3C 84. The brightness temperature analysis suggests that the system is in equipartition. We also determined a turnover frequency of νm = (113 ± 4) GHz, a corresponding synchrotron self-absorbed magnetic field of BSSA = (2.9 ± 1.6) G, and an equipartition magnetic field of Beq = (5.2 ± 0.6) G. Three components are resolved with the highest fractional polarisation detected for this object (mnet = (17.0 ± 3.9)%). The positions of the components are compatible with those seen in low-frequency VLBI observations since 2017-2018. We report a steeply negative slope of the spectrum at 228 GHz. We used these findings to test existing models of jet formation, propagation, and Faraday rotation in 3C 84.
Conclusions. The findings of our investigation into different flow geometries and black hole spins support an advection-dominated accretion flow in a magnetically arrested state around a rapidly rotating supermassive black hole as a model of the jet-launching system in the core of 3C 84. However, systematic uncertainties due to the limited (u, v)-coverage, however, cannot be ignored. Our upcoming work using new EHT data, which offer full imaging capabilities, will shed more light on the compact region of 3C 84.
Techniques: high angular resolution
Galaxies: individual: NGC 1275
Techniques: interferometric
Galaxies: jets
Galaxies: active
Författare
Georgios Filippos Paraschos
Max-Planck-Gesellschaft
M. Wielgus
Max-Planck-Gesellschaft
J. Röder
Max-Planck-Gesellschaft
T.P. Krichbaum
Max-Planck-Gesellschaft
Eduardo Ros
Max-Planck-Gesellschaft
I. Agudo
Instituto de Astrofisica de Andalucía (IAA)
I. Myserlis
Max-Planck-Gesellschaft
M. Mościbrodzka
Radboud Universiteit
E. Traianou
Max-Planck-Gesellschaft
A.J. Zensus
Max-Planck-Gesellschaft
Lindy Blackburn
Harvard University
Chi Kwan Chan
University of Arizona
S. Issaoun
Harvard-Smithsonian Center for Astrophysics
Michael Janssen
Max-Planck-Gesellschaft
Michael D. Johnson
Harvard University
V. Fish
Massachusetts Institute of Technology (MIT)
Kazunori Akiyama
Harvard University
Antxon Alberdi
Instituto de Astrofisica de Andalucía (IAA)
Walter Alef
Max-Planck-Gesellschaft
Juan-Carlos Algaba
University of Malaya
Richard Anantua
Harvard University
K. Asada
Academia Sinica
R. Azulay
Max-Planck-Gesellschaft
U. Bach
Max-Planck-Gesellschaft
David Ball
University of Arizona
Mislav Baloković
Yale University
John Barrett
Massachusetts Institute of Technology (MIT)
M. Bauböck
The Grainger College of Engineering
Bradford A. Benson
Fermi National Accelerator Laboratory
Dan Bintley
East Asian Observatory
R. Blundell
Harvard-Smithsonian Center for Astrophysics
K. L. Bouman
California Institute of Technology (Caltech)
G. C. Bower
Academia Sinica
Hope Boyce
McGill University
M. Bremer
Institut de Radioastronomie Millimétrique (IRAM)
C. D. Brinkerink
Radboud Universiteit
Roger Brissenden
Harvard University
Silke Britzen
Max-Planck-Gesellschaft
Avery E. Broderick
Perimeter Institute for Theoretical Physics
D. Broguière
Institut de Radioastronomie Millimétrique (IRAM)
Thomas Bronzwaer
Radboud Universiteit
Sandra Bustamente
University of Massachusetts
Do Young Byun
Korea Astronomy and Space Science Institute
J. E. Carlstrom
University of Chicago
Chiara Ceccobello
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
A. Chael
Princeton University
Dominic O. Chang
Harvard University
Koushik Chatterjee
Harvard University
S. Chatterjee
Cornell University
Ming Tang Chen
Academia Sinica
Yongjun Chen
Shanghai Astronomical Observatory
X. P. Cheng
Korea Astronomy and Space Science Institute
I. Cho
Instituto de Astrofisica de Andalucía (IAA)
Pierre Christian
Fairfield University
Nicholas S. Conroy
Harvard-Smithsonian Center for Astrophysics
John Conway
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
James M. Cordes
Cornell University
Thomas M. Crawford
University of Chicago
G. Crew
Massachusetts Institute of Technology (MIT)
Alejandro Cruz-Osorio
Universidad Nacional Autónoma de México
Yuzhu Cui
Zhejiang Lab
Rohan Dahale
Instituto de Astrofisica de Andalucía (IAA)
Jordy Davelaar
Radboud Universiteit
Mariafelicia De Laurentis
Johann Wolfgang Goethe Universität Frankfurt am Main
R. P. Deane
University of Witwatersrand
Jessica Dempsey
East Asian Observatory
Gregory Desvignes
Max-Planck-Gesellschaft
Jason Dexter
JILA
Vedant Dhruv
The Grainger College of Engineering
S. Doeleman
Harvard University
Sean Dougal
University of Arizona
Sergio A. Dzib
Max-Planck-Gesellschaft
Ralph P. Eatough
Max-Planck-Gesellschaft
Razieh Emami
Harvard-Smithsonian Center for Astrophysics
H.D. Falcke
Radboud Universiteit
Joseph R. Farah
Las Cumbres Observatory Global Telescope Network
E. Fomalont
National Radio Astronomy Observatory
H. Alyson Ford
University of Arizona
Marianna Foschi
Instituto de Astrofisica de Andalucía (IAA)
R. Fraga-Encinas
Radboud Universiteit
W.T. Freeman
Massachusetts Institute of Technology
P. Friberg
East Asian Observatory
Christian M. Fromm
Max-Planck-Gesellschaft
Antonio Fuentes
Instituto de Astrofisica de Andalucía (IAA)
Peter Galison
Harvard University
Charles F. Gammie
The Grainger College of Engineering
Roberto Garcia
Institut de Radioastronomie Millimétrique (IRAM)
Olivier Gentaz
Institut de Radioastronomie Millimétrique (IRAM)
Boris Georgiev
Perimeter Institute for Theoretical Physics
C. Goddi
Universidade de Sao Paulo (USP)
R. Gold
Syddansk Universitet
Arturo I. Gómez-Ruiz
Instituto Nacional de Astrofísica, Óptica y Electrońica
J. L. Gomez
Instituto de Astrofisica de Andalucía (IAA)
Minfeng Gu
Shanghai Astronomical Observatory
M. Gurwell
Harvard-Smithsonian Center for Astrophysics
K. Hada
National Astronomical Observatory of Japan
Daryl Haggard
McGill University
Kari Haworth
Harvard-Smithsonian Center for Astrophysics
Michael H. Hecht
Massachusetts Institute of Technology (MIT)
R. Hesper
Rijksuniversiteit Groningen
Dirk Heumann
University of Arizona
Luis C. Ho
Beijing University of Technology
P. T. P. Ho
Academia Sinica
M. Honma
National Astronomical Observatory of Japan
C.L. Huang
Academia Sinica
Lei Huang
Shanghai Astronomical Observatory
D. Hughes
Instituto Nacional de Astrofísica, Óptica y Electrońica
Shiro Ikeda
National Astronomical Observatory of Japan
C. M. V. Impellizzeri
National Radio Astronomy Observatory
Makoto Inoue
Academia Sinica
David J. James
ASTRAVEO
Buell T. Jannuzi
University of Arizona
Britton Jeter
Academia Sinica
W. Jaing
Shanghai Astronomical Observatory
Alejandra Jimenez-Rosales
Radboud Universiteit
S.G. Jorstad
Boston University
Abhishek V. Joshi
The Grainger College of Engineering
Taehyun Jung
Korea Astronomy and Space Science Institute
Mansour Karami
Perimeter Institute for Theoretical Physics
Tomohisa Kawashima
University of Tokyo
G. Keating
Harvard-Smithsonian Center for Astrophysics
M. M. Kettenis
Joint Institute for VLBI in Europe (JIVE)
D.-J. Kim
Max-Planck-Gesellschaft
Jae-Young Kim
Max-Planck-Gesellschaft
Junhan Kim
California Institute of Technology (Caltech)
Jae-Young Kim
Korea Astronomy and Space Science Institute
R. Karuppusamy
Max-Planck-Gesellschaft
R. Karuppusamy
National Astronomical Observatory of Japan
Jun Yi Koay
Academia Sinica
Prashant Kocherlakota
Johann Wolfgang Goethe Universität Frankfurt am Main
Yutaro Kofuji
National Astronomical Observatory of Japan
Patrick M. Koch
Academia Sinica
Shoko Koyama
Academia Sinica
C. Kramer
Institut de Radioastronomie Millimétrique (IRAM)
Joana A. Kramer
Max-Planck-Gesellschaft
M. Kramer
Max-Planck-Gesellschaft
Cheng Yu Kuo
Academia Sinica
Tod R. Lauer
National Optical Astronomy Observatory
Daeyoung Lee
The Grainger College of Engineering
Sang Sung Lee
Korea Astronomy and Space Science Institute
Po Kin Leung
Chinese University of Hong Kong
Aviad Levis
California Institute of Technology (Caltech)
Zhiyuan Li
Nanjing University
R. Lico
Instituto de Astrofisica de Andalucía (IAA)
Greg Lindahl
Harvard-Smithsonian Center for Astrophysics
Michael Lindqvist
Radboud Universiteit
Michael Lindqvist
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
Mikhail Lisakov
Max-Planck-Gesellschaft
Jun Liu
Max-Planck-Gesellschaft
Kuo Liu
Max-Planck-Gesellschaft
Elisabetta Liuzzo
Istituto di Radioastronomia
Wen-Ping Lo
Academia Sinica
A. P. Lobanov
Max-Planck-Gesellschaft
L. Loinard
Universidad Nacional Autónoma de México
Colin Lonsdale
Massachusetts Institute of Technology (MIT)
Amy E. Lowitz
University of Arizona
R.S. Lu
Max-Planck-Gesellschaft
N. R. Macdonald
Max-Planck-Gesellschaft
Jirong Mao
Yunnan Observatories
Nicola Marchili
Max-Planck-Gesellschaft
S. Markoff
Anton Pannekoek Institute for Astronomy
D. P. Marrone
University of Arizona
A. Marscher
Boston University
Ivan Marti-Vidal
Universitat de Valencia
S. Matsushita
Academia Sinica
Lynn D. Matthews
Massachusetts Institute of Technology (MIT)
Lia Medeiros
Einstein Fellow
K. Menten
Max-Planck-Gesellschaft
Daniel Michalik
University of Chicago
Izumi Mizuno
East Asian Observatory
Yosuke Mizuno
Johann Wolfgang Goethe Universität Frankfurt am Main
James M. Moran
Harvard University
Kotaro Moriyama
Massachusetts Institute of Technology (MIT)
Wanga Mulaudzi
Anton Pannekoek Institute for Astronomy
C. Müller
Max-Planck-Gesellschaft
Hendrik Müller
Max-Planck-Gesellschaft
A. Mus
Universitat de Valencia
Gibwa Musoke
Radboud Universiteit
Andrew Nadolski
University of Illinois
H. Nagai
National Astronomical Observatory of Japan
N. M. Nagar
Universidad de Concepción
Masanori Nakamura
Academia Sinica
Gopal Narayanan
University of Massachusetts
Iniyan Natarajan
Harvard University
Antonios Nathanail
Johann Wolfgang Goethe Universität Frankfurt am Main
S. Navarro Fuentes
Institut de Radioastronomie Millimétrique (IRAM)
Joseph Neilsen
Villanova University
R. Neri
Institut de Radioastronomie Millimétrique (IRAM)
Chunchong Ni
Perimeter Institute for Theoretical Physics
A. Noutsos
Max-Planck-Gesellschaft
Michael A. Nowak
Washington University in St. Louis
Junghwan Oh
Kogakuin University of Technology and Engineering
Hiroki Okino
National Astronomical Observatory of Japan
Héctor Olivares
Radboud Universiteit
G.N. Ortiz-León
Max-Planck-Gesellschaft
Tomoaki Oyama
National Astronomical Observatory of Japan
Feryal Özel
Georgia Institute of Technology
Daniel C.M. Palumbo
Harvard University
Jongho Park
Kyung Hee University
Harriet Parsons
East Asian Observatory
N. Patel
Harvard-Smithsonian Center for Astrophysics
U. L. Pen
Academia Sinica
Vincent Piétu
Institut de Radioastronomie Millimétrique (IRAM)
Richard L. Plambeck
University of California
Aleksandar PopStefanija
University of Massachusetts
Oliver Porth
Johann Wolfgang Goethe Universität Frankfurt am Main
Felix M. Pötzl
Max-Planck-Gesellschaft
Ben Prather
The Grainger College of Engineering
Jorge A. Preciado-López
Perimeter Institute for Theoretical Physics
Dimitrios Psaltis
Georgia Institute of Technology
Hung-Yi Pu
Academia Sinica
Venkatessh Ramakrishnan
Universidad de Concepción
R. Rao
Harvard-Smithsonian Center for Astrophysics
M.G. Rawlings
University of Chicago
Alexander W. Raymond
Harvard University
L. Rezzolla
Johann Wolfgang Goethe Universität Frankfurt am Main
Angelo Ricarte
Harvard University
Bart Ripperda
Perimeter Institute for Theoretical Physics
F. Roelofs
Radboud Universiteit
A.E.E. Rogers
Massachusetts Institute of Technology (MIT)
C. Romero-Cañizales
Academia Sinica
Arash Roshanineshat
University of Arizona
H. Rottmann
Max-Planck-Gesellschaft
A. Roy
Max-Planck-Gesellschaft
Ignacio Ruiz
Institut de Radioastronomie Millimétrique (IRAM)
C. Ruszczyk
Massachusetts Institute of Technology (MIT)
Kazi L.J. Rygl
Istituto di Radioastronomia
S. Sanchez
Institut de Radioastronomie Millimétrique (IRAM)
David Sánchez-Arguelles
Instituto Nacional de Astrofísica, Óptica y Electrońica
M. Sánchez Portal
Institut de Radioastronomie Millimétrique (IRAM)
Mahito Sasada
National Astronomical Observatory of Japan
Kaushik Satapathy
University of Arizona
Anne-Kathrin Baczko
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Max-Planck-Gesellschaft
T. Savolainen
Max-Planck-Gesellschaft
F. P. Schloerb
University of Massachusetts
Jonathan Schonfeld
Harvard-Smithsonian Center for Astrophysics
K. Schuster
Institut de Radioastronomie Millimétrique (IRAM)
Lijing Shao
Max-Planck-Gesellschaft
Zhi Qiang Shen
Shanghai Astronomical Observatory
Des Small
Joint Institute for VLBI in Europe (JIVE)
B. W. Sohn
Korea Astronomy and Space Science Institute
J. SooHoo
Massachusetts Institute of Technology (MIT)
León David Sosapanta Salas
Anton Pannekoek Institute for Astronomy
Kamal Souccar
University of Massachusetts
He Sun
Beijing University of Technology
Fumie Tazaki
National Astronomical Observatory of Japan
Alexandra J. Tetarenko
University of Lethbridge
Paul Tiede
Harvard University
R. P. J. Tilanus
Radboud Universiteit
M. Titus
Massachusetts Institute of Technology (MIT)
Pablo Torne
Max-Planck-Gesellschaft
Teresa Toscano
Instituto de Astrofisica de Andalucía (IAA)
Tyler Trent
University of Arizona
S. Trippe
Seoul National University
Matthew Turk
University of Illinois
I. van Bemmel
Kogakuin University of Technology and Engineering
H. J. van Langevelde
ASTRAVEO
Daniel R. van Rossum
Radboud Universiteit
Jesse Vos
Radboud Universiteit
Jan Wagner
Max-Planck-Gesellschaft
D. Ward-Thompson
University of Central Lancashire
John Wardle
Brandeis University
Jasmin E. Washington
University of Arizona
J. Weintroub
Harvard University
Robert Wharton
Max-Planck-Gesellschaft
K. Wiik
Tuorla Observatory
Gunther Witzel
Max-Planck-Gesellschaft
Michael F. Wondrak
Radboud Universiteit
George N. Wong
Princeton University
Qingwen Wu
Huazhong University of Science and Technology
Nitika Yadlapalli
California Institute of Technology (Caltech)
Paul Yamaguchi
Harvard-Smithsonian Center for Astrophysics
Aristomenis Yfantis
Radboud Universiteit
Doosoo Yoon
Anton Pannekoek Institute for Astronomy
A. Young
Radboud Universiteit
K. Young
Harvard-Smithsonian Center for Astrophysics
Ziri Younsi
Johann Wolfgang Goethe Universität Frankfurt am Main
Wei Yu
Harvard-Smithsonian Center for Astrophysics
F. Yuan
Shanghai Astronomical Observatory
Ye-Fei Yuan
University of Science and Technology of China
Shuo Zhang
Michigan State University
G. Y. Zhao
Instituto de Astrofisica de Andalucía (IAA)
Shan-Shan Zhao
Shanghai Astronomical Observatory
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 682 L3Ämneskategorier
Astronomi, astrofysik och kosmologi
Annan fysik
Fusion, plasma och rymdfysik
DOI
10.1051/0004-6361/202348308