MétaCan
Menu
Back to cohort
Record W4367050035 · doi:10.1038/s41586-023-05843-w

A ring-like accretion structure in M87 connecting its black hole and jet

2023· article· en· W4367050035 on OpenAlexafffund
Ru-Sen Lu, Keiichi Asada, T. P. Krichbaum, Jongho Park, Fumie Tazaki, Hung-Yi Pu, Masanori Nakamura, A. P. Lobanov, Kazuhiro Hada, Kazunori Akiyama, Jae-Young Kim, I. Martí‐Vidal, José L. Gómez, Tomohisa Kawashima, Ye‐Fei Yuan, E. Ros, W. Alef, S. Britzen, Michael Bremer, Avery E. Broderick, Akihiro Doi, G. Giovannini, M. Giroletti, Paul T. P. Ho, Mareki Honma, D. H. Hughes, Makoto Inoue, Motoki Kino, Shoko Koyama, M. Lindqvist, Alan P. Marscher, Satoki Matsushita, Hiroshi Nagai, Helge Rottmann, T. Savolainen, K. Schüster, Zhi-Qiang Shen, P. de Vicente, R. C. Walker, Hai Yang, J. A. Zensus, Juan Carlos Algaba, Alexander Allardi, U. Bach, Ryan Berthold, Dan Bintley, Do‐Young Byun, C. Casadio, Shu-Hao Chang, Chih-Cheng Chang, Song-Chu Chang, Chung-Chen Chen, Ming‐Tang Chen, Ryan Chilson, Tim C. Chuter, J. E. Conway, G. Crew, Jessica Dempsey, Sven Dornbusch, Aaron Faber, Per Friberg, Javier González-García, M. Gómez-Garrido, Chih-Chiang Han, Kuo-Chang Han, Yutaka Hasegawa, R. Herrero‐Illana, Teddy Huang, C. M. Violette Impellizzeri, Homin Jiang, H. Jinchi, Taehyun Jung, J. Kallunki, Petri Kirves, Kimihiro Kimura, Jun Yi Koay, Patrick M. Koch, C. Krämer, Alex Kraus, Derek Kubo, Cheng‐Yu Kuo, Chao-Te Li, L. C.-C. Lin, Ching-Tang Liu, Kuan-Yu Liu, Wen-Ping Lo, Li-Ming Lu, Nicholas R. MacDonald, Pierre Martin-Cocher, Hugo Messias, Zheng Meyer-Zhao, Anthony H. Minter, Dhanya G. Nair, Hiroaki Nishioka, Timothy Norton, George Nystrom, Hideo Ogawa, Peter Oshiro, Nimesh Patel, Ue‐Li Pen, Yurii Pidopryhora, Nicolas Pradel, Philippe Raffin, Ramprasad Rao, Ignacio Ruiz, Salvador Sánchez, Paul Shaw, W. M. Snow, T. K. Sridharan, Ranjani Srinivasan, B. Tercero, Pablo Torné, Efthalia Traianou, Jan Wagner, Craig Walther, Ta-Shun Wei, Jun Yang, Chen-Yu Yu

Bibliographic record

VenueNature · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsWestern UniversityPerimeter InstituteUniversity of Waterloo
FundersJapan Society for the Promotion of ScienceSmithsonian Astrophysical ObservatoryInstitut Périmètre de physique théoriqueChinese Academy of Sciences, Shanghai BranchMinistero dello Sviluppo EconomicoNational Astronomical Observatory of JapanNational Institutes of Natural SciencesNuclear Safety and Security CommissionSmithsonian InstitutionNational Radio Astronomy ObservatoryNational Natural Science Foundation of ChinaVetenskapsrådetGeneralitat ValencianaNatural Sciences and Engineering Research Council of CanadaMinistry of Science and Technology, TaiwanMinistry of Education, IndiaPhysics Division, National Center for Theoretical SciencesAalto-YliopistoCentre National de la Recherche ScientifiqueChinese Academy of SciencesAcademy of FinlandNational Research FoundationAcademia SinicaMinisterio de Ciencia e InnovaciónEuropean CommissionMax-Planck-GesellschaftNational Center for Theoretical SciencesEast Asian Core Observatories AssociationInnovation, Science and Economic Development CanadaMinistry of Education, Culture, Sports, Science and TechnologyKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationGovernment of CanadaNational Science Foundation
KeywordsPhysicsAstrophysicsAccretion (finance)Black hole (networking)Schwarzschild radiusActive galactic nucleusJet (fluid)GalaxyEvent horizonSupermassive black holeAstronomyIntermediate-mass black holeWavelengthStellar black holeSpin-flipEvent (particle physics)Optics

Abstract

fetched live from OpenAlex

Abstract The nearby radio galaxy M87 is a prime target for studying black hole accretion and jet formation 1,2 . Event Horizon Telescope observations of M87 in 2017, at a wavelength of 1.3 mm, revealed a ring-like structure, which was interpreted as gravitationally lensed emission around a central black hole 3 . Here we report images of M87 obtained in 2018, at a wavelength of 3.5 mm, showing that the compact radio core is spatially resolved. High-resolution imaging shows a ring-like structure of $${8.4}_{-1.1}^{+0.5}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msubsup> <mml:mrow> <mml:mn>8.4</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1.1</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.5</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> Schwarzschild radii in diameter, approximately 50% larger than that seen at 1.3 mm. The outer edge at 3.5 mm is also larger than that at 1.3 mm. This larger and thicker ring indicates a substantial contribution from the accretion flow with absorption effects, in addition to the gravitationally lensed ring-like emission. The images show that the edge-brightened jet connects to the accretion flow of the black hole. Close to the black hole, the emission profile of the jet-launching region is wider than the expected profile of a black-hole-driven jet, suggesting the possible presence of a wind associated with the accretion flow.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.335
Threshold uncertainty score0.378

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.011
GPT teacher head0.254
Teacher spread0.243 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations143
Published2023
Admission routes2
Has abstractyes

Explore more

Same venueNatureSame topicAstrophysical Phenomena and ObservationsFrench-language works237,207