Issue |
A&A
Volume 693, January 2025
|
|
---|---|---|
Article Number | A265 | |
Number of page(s) | 27 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/202451296 | |
Published online | 22 January 2025 |
The persistent shadow of the supermassive black hole of M87
II. Model comparisons and theoretical interpretations
1
Massachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA, 01886, USA
2
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan
3
Black Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA, 02138, USA
4
Departament d’Astronomia i Astrofísica, Universitat de València, C. Dr. Moliner 50, E-46100 Burjassot, València, Spain
5
Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, Spain
6
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
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Department of Physics, Faculty of Science, Universiti Malaya, 50603 Kuala Lumpur, Malaysia
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Department of Physics & Astronomy, The University of Texas at San Antonio, One UTSA Circle, San Antonio, TX, 78249, USA
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Physics & Astronomy Department, Rice University, Houston, TX, 77005-1827, USA
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Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA, 02138, USA
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Institute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd., Taipei, 106216, Taiwan, ROC
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Observatori Astronòmic, Universitat de València, C. Catedrático José Beltrán 2, E-46980 Paterna, València, Spain
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Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala, Sweden
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Steward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ, 85721, USA
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Yale Center for Astronomy & Astrophysics, Yale University, 52 Hillhouse Avenue, New Haven, CT, 06511, USA
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Astronomy Department, Universidad de Concepción, Casilla 160-C, Concepción, Chile
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Department of Physics, University of Illinois, 1110 West Green Street, Urbana, IL, 61801, USA
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Program in Applied Mathematics, University of Arizona, 617 N. Santa Rita, Tucson, AZ, 85721, USA
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Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY, 14853, USA
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Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030, PR China
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Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing, 100101, PR China
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Korea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon, 34055, Republic of Korea
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Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL, 61801, USA
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Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shengrong Road 520, Shanghai, 201210, People’s Republic of China
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Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ, 08544, USA
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Dipartimento di Fisica “E. Pancini”, Università di Napoli “Federico II”, Compl. Univ. di Monte S. Angelo, Edificio G, Via Cinthia, I-80126 Napoli, Italy
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57
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Department of Physics, University of California, Santa Barbara, CA, 93106-9530, USA
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Department of Physics, Harvard University, Cambridge, MA, 02138, USA
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Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, R. do Matão, 1226, São Paulo, SP, 05508-090, Brazil
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69
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Graduate School of Science, Nagoya City University, Yamanohata 1, Mizuho-cho, Mizuho-ku, Nagoya, 467-8501 Aichi, Japan
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Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate, 023-0861, Japan
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Department of Astronomical Science, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan
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Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
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87
Department of Statistical Science, The Graduate University for Advanced Studies (SOKENDAI), 10-3 Midori-cho, Tachikawa, Tokyo, 190-8562, Japan
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University of Science and Technology, Gajeong-ro 217, Yuseong-gu, Daejeon, 34113, Republic of Korea
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Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba, 277-8582, Japan
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Joint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands
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School of Physics and Astronomy, Shanghai Jiao Tong University, 800 Dongchuan Road, Shanghai, 200240, PR China
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Institut de Radioastronomie Millimétrique (IRAM), Avenida Divina Pastora 7, Local 20, E-18012 Granada, Spain
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National Institute of Technology, Hachinohe College, 16-1 Uwanotai, Tamonoki, Hachinohe City, Aomori, 039-1192, Japan
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School of Space Research, Kyung Hee University, 1732, Deogyeong-daero, Giheung-gu, Yongin-si, Gyeonggi-do, 17104, Republic of Korea
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Astronomical Institute, Tohoku University, Sendai, 980-8578, Japan
148
Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul, 08826, Republic of Korea
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University of New Mexico, Department of Physics and Astronomy, Albuquerque, NM, 87131, USA
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Physics Department, Brandeis University, 415 South Street, Waltham, MA, 02453, USA
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Tuorla Observatory, Department of Physics and Astronomy, University of Turku, FI-20014 Turun Yliopisto, Finland
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School of Physics, Huazhong University of Science and Technology, Wuhan, Hubei, 430074, PR China
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Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK
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Center for Astronomy and Astrophysics and Department of Physics, Fudan University, Shanghai, 200438, PR China
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Astronomy Department, University of Science and Technology of China, Hefei, 230026, PR China
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Department of Physics and Astronomy, Michigan State University, 567 Wilson Rd, East Lansing, MI, 48824, USA
⋆⋆⋆ Corresponding author; ehtrepository@gmail.com
Received:
28
June
2024
Accepted:
8
October
2024
The Event Horizon Telescope (EHT) observation of M87∗ in 2018 has revealed a ring with a diameter that is consistent with the 2017 observation. The brightest part of the ring is shifted to the southwest from the southeast. In this paper, we provide theoretical interpretations for the multi-epoch EHT observations for M87∗ by comparing a new general relativistic magnetohydrodynamics model image library with the EHT observations for M87∗ in both 2017 and 2018. The model images include aligned and tilted accretion with parameterized thermal and nonthermal synchrotron emission properties. The 2018 observation again shows that the spin vector of the M87∗ supermassive black hole is pointed away from Earth. A shift of the brightest part of the ring during the multi-epoch observations can naturally be explained by the turbulent nature of black hole accretion, which is supported by the fact that the more turbulent retrograde models can explain the multi-epoch observations better than the prograde models. The EHT data are inconsistent with the tilted models in our model image library. Assuming that the black hole spin axis and its large-scale jet direction are roughly aligned, we expect the brightest part of the ring to be most commonly observed 90 deg clockwise from the forward jet. This prediction can be statistically tested through future observations.
Key words: accretion, accretion disks / black hole physics / gravitation / galaxies: active / galaxies: individual: M87 / galaxies: jets
© The Authors 2025
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