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First Sagittarius A...
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Akiyama, KazunoriMassachusetts Institute of Technology (MIT)
(author)
First Sagittarius A∗ Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring
- Article/chapterEnglish2024
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2024
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electronicrdacarrier
Numbers
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LIBRIS-ID:oai:research.chalmers.se:6fca8793-1c65-4b35-8ded-f1ace452f038
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https://doi.org/10.3847/2041-8213/ad2df1DOI
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https://research.chalmers.se/publication/540716URI
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Language:English
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Summary in:English
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Subject category:art swepub-publicationtype
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Subject category:ref swepub-contenttype
Notes
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In a companion paper, we present the first spatially resolved polarized image of Sagittarius A∗ on event horizon scales, captured using the Event Horizon Telescope, a global very long baseline interferometric array operating at a wavelength of 1.3 mm. Here we interpret this image using both simple analytic models and numerical general relativistic magnetohydrodynamic (GRMHD) simulations. The large spatially resolved linear polarization fraction (24%-28%, peaking at ∼40%) is the most stringent constraint on parameter space, disfavoring models that are too Faraday depolarized. Similar to our studies of M87∗, polarimetric constraints reinforce a preference for GRMHD models with dynamically important magnetic fields. Although the spiral morphology of the polarization pattern is known to constrain the spin and inclination angle, the time-variable rotation measure (RM) of Sgr A∗ (equivalent to ≈ 46° ± 12° rotation at 228 GHz) limits its present utility as a constraint. If we attribute the RM to internal Faraday rotation, then the motion of accreting material is inferred to be counterclockwise, contrary to inferences based on historical polarized flares, and no model satisfies all polarimetric and total intensity constraints. On the other hand, if we attribute the mean RM to an external Faraday screen, then the motion of accreting material is inferred to be clockwise, and one model passes all applied total intensity and polarimetric constraints: a model with strong magnetic fields, a spin parameter of 0.94, and an inclination of 150°. We discuss how future 345 GHz and dynamical imaging will mitigate our present uncertainties and provide additional constraints on the black hole and its accretion flow.
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Alberdi, AntxonInstituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)
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Schloerb, F. P.University of Massachusetts
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Schonfeld, JonathanHarvard-Smithsonian Center for Astrophysics
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Schuster, K.Institut de Radioastronomie Millimétrique (IRAM)
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Sun, HeBeijing University of Technology
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Tiede, PaulHarvard University
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Torne, PabloMax Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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Trent, TylerUniversity of Arizona
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Trippe, S.Seoul National University
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Turk, MatthewUniversity of Illinois
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van Bemmel, I.Joint Institute for VLBI in Europe (JIVE)
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van Langevelde, H. J.Universiteit Leiden (UL),Leiden University (UL)
(author)
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van Rossum, Daniel R.Radboud Universiteit,Radboud University
(author)
-
Vos, JesseRadboud Universiteit,Radboud University
(author)
-
Wagner, JanMax Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
(author)
-
Ward-Thompson, D.University of Central Lancashire
(author)
-
Wardle, JohnBrandeis University
(author)
-
Washington, Jasmin E.University of Arizona
(author)
-
Weintroub, J.Harvard University
(author)
-
Wharton, RobertMax Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
(author)
-
Wielgus, M.Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
(author)
-
Wiik, K.
(author)
-
Witzel, GuntherMax Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
(author)
-
Wondrak, Michael F.Radboud Universiteit,Radboud University
(author)
-
Wong, George N.Princeton University
(author)
-
Wu, QingwenHuazhong University of Science and Technology
(author)
-
Yadlapalli, NitikaCalifornia Institute of Technology (Caltech)
(author)
-
Yamaguchi, PaulHarvard-Smithsonian Center for Astrophysics
(author)
-
Yfantis, AristomenisRadboud Universiteit,Radboud University
(author)
-
Yoon, DoosooAnton Pannekoek Institute for Astronomy
(author)
-
Young, A.Radboud Universiteit,Radboud University
(author)
-
Young, KenHarvard-Smithsonian Center for Astrophysics
(author)
-
Younsi, ZiriJohann Wolfgang Goethe Universität Frankfurt am Main,Goethe University Frankfurt
(author)
-
Yu, WeiHarvard-Smithsonian Center for Astrophysics
(author)
-
Yuan, FengFudan University
(author)
-
Yuan, Ye-FeiUniversity of Science and Technology of China
(author)
-
Zensus, A.Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
(author)
-
Zhang, ShuoMichigan State University
(author)
-
Zhao, G. Y.Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)
(author)
-
Zhao, Shan-ShanShanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences
(author)
-
Najafi-Ziyazi, MahdiAnton Pannekoek Institute for Astronomy
(author)
-
Massachusetts Institute of Technology (MIT)Instituto de Astrofisica de Andalucía (IAA)
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