First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring

doi:10.3847/2041-8213/ad2df1

CORC > 云南天文台 > 中国科学院云南天文台 > 中国科学院天体结构与演化重点实验室

	*First Sagittarius A Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring**
	Akiyama, Kazunori 150,151,152; Alberdi, Antxon 149; Alef, Walter 148; Algaba, Juan Carlos 147; Anantua, Richard 145,146,150; Asada, Keiichi 144; Azulay, Rebecca 142,143,148; Bach, Uwe 148; Baczko, Anne-Kathrin 141,148; Ball, David 140
刊名	ASTROPHYSICAL JOURNAL LETTERS
	2024-04-01
卷号	964 期号:2
ISSN号	2041-8205
DOI	10.3847/2041-8213/ad2df1
产权排序	第107完成单位
文献子类	Article
英文摘要	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 similar to 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 approximate to 46 degrees +/- 12 degrees 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 degrees. 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.
学科主题	天文学 ; 星系与宇宙学
URL标识	查看原文
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
资助项目	Academia Sinica; Academy of Finland[274477]; Academy of Finland[284495]; Academy of Finland[312496]; Academy of Finland[315721]; Agencia Nacional de Investigacion y Desarrollo (ANID), Chile[NCN19_058]; Fondecyt[1221421]; BASAL[FB210003]; Alexander von Humboldt Stiftung; Alfred P. Sloan Research Fellowship; European ALMA Regional Centre node in the Netherlands; NL astronomy research network NOVA; Allegro; University of Amsterdam; Leiden University; Radboud University; ALMA North America Development Fund; Astrophysics and High Energy Physics program by MCIN (European Union NextGenerationEU)[PRTR-C17I1]; Black Hole Initiative - John Templeton Foundation[60477]; Black Hole Initiative - John Templeton Foundation[61497]; Black Hole Initiative - John Templeton Foundation[62286]; Gordon and Betty Moore Foundation[GBMF-8273]; Brinson Foundation; la Caixa Foundation[100010434]; la Caixa Foundation[LCF/BQ/DI22/11940027]; la Caixa Foundation[LCF/BQ/DI22/11940030]; la Caixa Foundation[DD7-18089X]; la Caixa Foundation[TM6-17006X]; China Scholarship Council; China Postdoctoral Science Foundation[2020M671266]; China Postdoctoral Science Foundation[2022M712084]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[U0004-246083]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[U0004-259839]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[F0003-272050]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[M0037-279006]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[F0003-281692]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[104497]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[275201]; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[263356]; Colfuturo Scholarship; Consejeria de Economia, Conocimiento, Empresas y Universidad of the Junta de Andalucia[P18-FR-1769]; Consejo Superior de Investigaciones Cientificas[2019AEP112]; Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN112820]; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN108324]; Dutch Organization for Scientific Research (NWO)[639.043.513]; Dutch Organization for Scientific Research (NWO)[OCENW.KLEIN.113]; Dutch Black Hole Consortium of the research program the National Science Agenda[NWA 1292.19.202]; Dutch National Supercomputers, Cartesius and Snellius (NWO)[2021.013]; EACOA Fellowship - East Asia Core Observatories Association; Academia Sinica Institute of Astronomy and Astrophysics; National Astronomical Observatory of Japan; Center for Astronomical Mega-Science, Chinese Academy of Sciences; Korea Astronomy and Space Science Institute; European Research Council (ERC) Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058]; European Union's Horizon 2020 research and innovation program[730562]; European Union's Horizon 2020 research and innovation program[101018682]; Horizon ERC Grants 2021 program[101040021]; European Research Council[884631]; FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)[2021/01183-8]; Fondo CAS-ANID folio[CAS220010]; Generalitat Valenciana[APOSTD/2018/177]; Generalitat Valenciana[ASFAE/2022/018]; GenT Program[CIDEGENT/2018/021]; A Gordon and Betty Moore Foundation[GBMF-3561]; A Gordon and Betty Moore Foundation[GBMF-5278]; A Gordon and Betty Moore Foundation[GBMF-10423]; Institute for Advanced Study; Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEON-GRAV; International Max Planck Research School for Astronomy and Astrophysics at the Universities of Bonn and Cologne; DFG research grant Jet physics on horizon scales and beyond[443220636]; Joint Columbia/Flatiron Postdoctoral Fellowship (Simons Foundation); Japan Ministry of Education, Culture, Sports, Science and Technology (MEXT)[JPMXP1020200109]; Japan Society for the Promotion of Science (JSPS)[JP17J08829]; Joint Institute for Computational Fundamental Science, Japan; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH057]; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SYS008]; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[ZDBS-LY-SLH011]; Leverhulme Trust Early Career Research Fellowship; Max-Planck-Gesellschaft (MPG); Max Planck Partner Group of the MPG; CAS; MEXT/JSPS KAKENHI[18KK0090]; MEXT/JSPS KAKENHI[JP21H01137]; MEXT/JSPS KAKENHI[JP18H03721]; MEXT/JSPS KAKENHI[JP18K13594]; MEXT/JSPS KAKENHI[18K03709]; MEXT/JSPS KAKENHI[JP19K14761]; MEXT/JSPS KAKENHI[18H01245]; MEXT/JSPS KAKENHI[25120007]; MEXT/JSPS KAKENHI[23K03453]; MICINN Research Projects[PID2019-108995GB-C22]; MICINN Research Projects[PID2022-140888NB-C22]; MIT International Science and Technology Initiatives (MISTI) Funds; Ministry of Science and Technology (MOST) of Taiwan[103-2119-M-001-010-MY2]; Ministry of Science and Technology (MOST) of Taiwan[105-2112-M-001-025-MY3]; Ministry of Science and Technology (MOST) of Taiwan[105-2119-M-001-042]; Ministry of Science and Technology (MOST) of Taiwan[106-2112-M-001-011]; Ministry of Science and Technology (MOST) of Taiwan[106-2119-M-001-013]; Ministry of Science and Technology (MOST) of Taiwan[106-2119-M-001-027]; Ministry of Science and Technology (MOST) of Taiwan[106-2923-M-001-005]; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-017]; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-020]; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001041]; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-110-005]; A Ministry of Science and Technology (MOST) of Taiwan[107-2923-M-001-009]; A Ministry of Science and Technology (MOST) of Taiwan[108-2112-M-001-048]; A Ministry of Science and Technology (MOST) of Taiwan[108-2112-M-001-051]; A Ministry of Science and Technology (MOST) of Taiwan[108-2923-M-001-002]; A Ministry of Science and Technology (MOST) of Taiwan[109-2112M-001-025]; A Ministry of Science and Technology (MOST) of Taiwan[109-2124-M-001-005]; A Ministry of Science and Technology (MOST) of Taiwan[109-2923-M-001-001]; A Ministry of Science and Technology (MOST) of Taiwan[1102112-M-003-007-MY2]; A Ministry of Science and Technology (MOST) of Taiwan[110-2112-M-001-033]; A Ministry of Science and Technology (MOST) of Taiwan[110-2124-M-001007]; A Ministry of Science and Technology (MOST) of Taiwan[110-2923-M-001-001]; Ministry of Education (MoE) of Taiwan Yushan Young Scholar Program; Physics Division, National Center for Theoretical Sciences of Taiwan; National Aeronautics and Space Administration (NASA)[80NSSC20K1567]; National Aeronautics and Space Administration (NASA)[80NSSC20K0527]; National Aeronautics and Space Administration (NASA)[80NSSC20K0645]; NASA Hubble Fellowship grants - Space Telescope Science Institute[HST-HF251431.001-A]; NASA Hubble Fellowship grants - Space Telescope Science Institute[HST-HF2-51482.001-A]; NASA[NAS5-26555]; National Institute of Natural Sciences (NINS) of Japan; National Key Research and Development Program of China[2016YFA0400704]; National Key Research and Development Program of China[2017YFA0402703]; National Key Research and Development Program of China[2016YFA0400702]; National Science and Technology Council (NSTC)[NSTC 111-2112-M-001-041]; National Science and Technology Council (NSTC)[NSTC 111-2124-M001-005]; National Science and Technology Council (NSTC)[NSTC 112-2124-M-001-014]; US National Science Foundation (NSF)[AST-0096454]; US National Science Foundation (NSF)[AST-0352953]; US National Science Foundation (NSF)[AST-0521233]; US National Science Foundation (NSF)[AST-0705062]; US National Science Foundation (NSF)[AST-0905844]; US National Science Foundation (NSF)[AST-0922984]; US National Science Foundation (NSF)[AST-1126433]; US National Science Foundation (NSF)[OIA-1126433]; US National Science Foundation (NSF)[AST-1140030]; US National Science Foundation (NSF)[DGE-1144085]; US National Science Foundation (NSF)[AST-1207704]; US National Science Foundation (NSF)[AST-1207730]; US National Science Foundation (NSF)[AST-1207752]; US National Science Foundation (NSF)[MRI-1228509]; US National Science Foundation (NSF)[OPP-1248097]; US National Science Foundation (NSF)[AST-1310896]; US National Science Foundation (NSF)[AST-1440254]; US National Science Foundation (NSF)[AST-1555365]; US National Science Foundation (NSF)[AST-1614868]; US National Science Foundation (NSF)[AST-1615796]; US National Science Foundation (NSF)[AST-1715061]; US National Science Foundation (NSF)[AST-1716327]; A US National Science Foundation (NSF)[AST-1726637]; A US National Science Foundation (NSF)[OISE-1743747]; A US National Science Foundation (NSF)[AST-1743747]; A US National Science Foundation (NSF)[AST-1816420]; A US National Science Foundation (NSF)[AST1952099]; A US National Science Foundation (NSF)[AST-1935980]; A US National Science Foundation (NSF)[AST-2034306]; A US National Science Foundation (NSF)[AST-2205908]; A US National Science Foundation (NSF)[AST2307887]; NSF Astronomy and Astrophysics Postdoctoral Fellowship[AST-1903847]; Natural Science Foundation of China[11650110427]; Natural Science Foundation of China[10625314]; Natural Science Foundation of China[11721303]; Natural Science Foundation of China[11725312]; Natural Science Foundation of China[11873028]; Natural Science Foundation of China[11933007]; Natural Science Foundation of China[11991052]; Natural Science Foundation of China[11991053]; Natural Science Foundation of China[12192220]; Natural Science Foundation of China[12192223]; Natural Science Foundation of China[12273022]; Natural Science Foundation of China[12325302]; Natural Science Foundation of China[12303021]; Natural Sciences and Engineering Research Council of Canada (NSERC); National Youth Thousand Talents Program of China; National Research Foundation of Korea[NRF-2015H1A2A1033752]; Korea Research Fellowship Program[NRF-2015H1D3A1066561]; Korea Research Fellowship Program[2019H1D3A1A01102564]; Korea Research Fellowship Program[2019R1F1A1059721]; Korea Research Fellowship Program[2021R1A6A3A01086420]; Korea Research Fellowship Program[2022R1C1C1005255]; Korea Research Fellowship Program[2022R1F1A1075115]; Netherlands Research School for Astronomy (NOVA) Virtual Institute of Accretion (VIA) postdoctoral fellowships; NOIRLab; Swedish Research Council[2017-00648]; Perimeter Institute for Theoretical Physic (Government of Canada through the Department of Innovation, Science and Economic Development); Perimeter Institute for Theoretical Physic (Province of Ontario through the Ministry of Research, Innovation and Science); Princeton Gravity Initiative; Spanish Ministerio de Ciencia e Innovacion[PGC2018-098915-B-C21]; Spanish Ministerio de Ciencia e Innovacion[AYA2016-80889-P]; Spanish Ministerio de Ciencia e Innovacion[PID2019-108995GB-C21]; Spanish Ministerio de Ciencia e Innovacion[PID2020-117404GB-C21]; University of Pretoria; Shanghai Municipality orientation program of basic research for international scientists[22JC1410600]; Shanghai Pilot Program for Basic Research, Chinese Academy of Science, Shanghai Branch[JCYJ-SHFY-2021-013]; State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa[SEV-2017-0709]; Spanish Ministry for Science and Innovation - MCIN/AEI[CEX2021-001131-S]; Spinoza Prize[SPI 78-409]; South African Research Chairs Initiative, through the South African Radio Astronomy Observatory (SARAO)[77948]; Toray Science Foundation; Swedish Research Council (VR); UK Science and Technology Facilities Council[ST/X508329/1]; US Department of Energy (USDOE) through the Los Alamos National Laboratory; National Nuclear Security Administration of the USDOE[89233218CNA000001]; YCAA Prize Postdoctoral Fellowship; Office of Science of the U.S. Department of Energy[DE-AC05-00OR22725]; ASTROVIVES FEDER infrastructure[IDIFEDER-2021-086]; Special Fund for Astronomy from the Ministry of Finance in China; A FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)[2021/01183-8]; Smithsonian Institution; A National Key Research and Development Program of China[2017YFA0402700]; A Natural Science Foundation of China[11873028]; A Natural Science Foundation of China[2030508]; A Natural Science Foundation of China[1836650]; Kavli Institute of Cosmological Physics at the University of Chicago; NSF[ACI-1548562]; NSF[DBI-0735191 DBI1265383 DBI-1743442]; Conicyt[QUIMAL170001]; Conicyt[PIA ACT172033]; A Fondecyt[11170268]; A Fondecyt[220002]; Compute Ontario; Calcul Quebec; Compute Canada
WOS关键词	ADVECTION-DOMINATED ACCRETION ; RELATIVISTIC MAGNETOHYDRODYNAMIC SIMULATIONS ; MAGNETICALLY ARRESTED ACCRETION ; ADAPTIVE MESH REFINEMENT ; BLACK-HOLE ; GRMHD SIMULATIONS ; OBSERVATIONAL SIGNATURES ; POLARIMETRIC IMAGES ; FARADAY-ROTATION ; ORBITAL MOTION
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP Publishing Ltd
WOS记录号	WOS:001194938600001
资助机构	Academia Sinica ; Academy of Finland[274477, 284495, 312496, 315721] ; Agencia Nacional de Investigacion y Desarrollo (ANID), Chile[NCN19_058] ; Fondecyt[1221421] ; BASAL[FB210003] ; Alexander von Humboldt Stiftung ; Alfred P. Sloan Research Fellowship ; European ALMA Regional Centre node in the Netherlands ; NL astronomy research network NOVA ; Allegro ; University of Amsterdam ; Leiden University ; Radboud University ; ALMA North America Development Fund ; Astrophysics and High Energy Physics program by MCIN (European Union NextGenerationEU)[PRTR-C17I1] ; Black Hole Initiative - John Templeton Foundation[60477, 61497, 62286] ; Gordon and Betty Moore Foundation[GBMF-8273] ; Brinson Foundation ; la Caixa Foundation[100010434, LCF/BQ/DI22/11940027, LCF/BQ/DI22/11940030, DD7-18089X, TM6-17006X] ; China Scholarship Council ; China Postdoctoral Science Foundation[2020M671266, 2022M712084] ; Consejo Nacional de Humanidades, Ciencia y Tecnologia (CONAHCYT, Mexico)[U0004-246083, U0004-259839, F0003-272050, M0037-279006, F0003-281692, 104497, 275201, 263356] ; Colfuturo Scholarship ; Consejeria de Economia, Conocimiento, Empresas y Universidad of the Junta de Andalucia[P18-FR-1769] ; Consejo Superior de Investigaciones Cientificas[2019AEP112] ; Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute ; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN112820, IN108324] ; Dutch Organization for Scientific Research (NWO)[639.043.513, OCENW.KLEIN.113] ; Dutch Black Hole Consortium of the research program the National Science Agenda[NWA 1292.19.202] ; Dutch National Supercomputers, Cartesius and Snellius (NWO)[2021.013] ; EACOA Fellowship - East Asia Core Observatories Association ; Academia Sinica Institute of Astronomy and Astrophysics ; National Astronomical Observatory of Japan ; Center for Astronomical Mega-Science, Chinese Academy of Sciences ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058] ; European Union's Horizon 2020 research and innovation program[730562, 101018682] ; Horizon ERC Grants 2021 program[101040021] ; European Research Council[884631] ; FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)[2021/01183-8] ; Fondo CAS-ANID folio[CAS220010] ; Generalitat Valenciana[APOSTD/2018/177, ASFAE/2022/018] ; GenT Program[CIDEGENT/2018/021] ; A Gordon and Betty Moore Foundation[GBMF-3561, GBMF-5278, GBMF-10423] ; Institute for Advanced Study ; Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEON-GRAV ; International Max Planck Research School for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; DFG research grant Jet physics on horizon scales and beyond[443220636] ; Joint Columbia/Flatiron Postdoctoral Fellowship (Simons Foundation) ; Japan Ministry of Education, Culture, Sports, Science and Technology (MEXT)[JPMXP1020200109] ; Japan Society for the Promotion of Science (JSPS)[JP17J08829] ; Joint Institute for Computational Fundamental Science, Japan ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH057, QYZDJ-SSW-SYS008, ZDBS-LY-SLH011] ; Leverhulme Trust Early Career Research Fellowship ; Max-Planck-Gesellschaft (MPG) ; Max Planck Partner Group of the MPG ; CAS ; MEXT/JSPS KAKENHI[18KK0090, JP21H01137, JP18H03721, JP18K13594, 18K03709, JP19K14761, 18H01245, 25120007, 23K03453] ; MICINN Research Projects[PID2019-108995GB-C22, PID2022-140888NB-C22] ; MIT International Science and Technology Initiatives (MISTI) Funds ; Ministry of Science and Technology (MOST) of Taiwan[103-2119-M-001-010-MY2, 105-2112-M-001-025-MY3, 105-2119-M-001-042, 106-2112-M-001-011, 106-2119-M-001-013, 106-2119-M-001-027, 106-2923-M-001-005, 107-2119-M-001-017, 107-2119-M-001-020, 107-2119-M-001041, 107-2119-M-110-005] ; A Ministry of Science and Technology (MOST) of Taiwan[107-2923-M-001-009, 108-2112-M-001-048, 108-2112-M-001-051, 108-2923-M-001-002, 109-2112M-001-025, 109-2124-M-001-005, 109-2923-M-001-001, 1102112-M-003-007-MY2, 110-2112-M-001-033, 110-2124-M-001007, 110-2923-M-001-001] ; Ministry of Education (MoE) of Taiwan Yushan Young Scholar Program ; Physics Division, National Center for Theoretical Sciences of Taiwan ; National Aeronautics and Space Administration (NASA)[80NSSC20K1567, 80NSSC20K0527, 80NSSC20K0645] ; NASA Hubble Fellowship grants - Space Telescope Science Institute[HST-HF251431.001-A, HST-HF2-51482.001-A] ; NASA[NAS5-26555] ; National Institute of Natural Sciences (NINS) of Japan ; National Key Research and Development Program of China[2016YFA0400704, 2017YFA0402703, 2016YFA0400702] ; National Science and Technology Council (NSTC)[NSTC 111-2112-M-001-041, NSTC 111-2124-M001-005, NSTC 112-2124-M-001-014] ; US National Science Foundation (NSF)[AST-0096454, AST-0352953, AST-0521233, AST-0705062, AST-0905844, AST-0922984, AST-1126433, OIA-1126433, AST-1140030, DGE-1144085, AST-1207704, AST-1207730, AST-1207752, MRI-1228509, OPP-1248097, AST-1310896, AST-1440254, AST-1555365, AST-1614868, AST-1615796, AST-1715061, AST-1716327] ; A US National Science Foundation (NSF)[AST-1726637, OISE-1743747, AST-1743747, AST-1816420, AST1952099, AST-1935980, AST-2034306, AST-2205908, AST2307887] ; NSF Astronomy and Astrophysics Postdoctoral Fellowship[AST-1903847] ; Natural Science Foundation of China[11650110427, 10625314, 11721303, 11725312, 11873028, 11933007, 11991052, 11991053, 12192220, 12192223, 12273022, 12325302, 12303021] ; Natural Sciences and Engineering Research Council of Canada (NSERC) ; National Youth Thousand Talents Program of China ; National Research Foundation of Korea[NRF-2015H1A2A1033752] ; Korea Research Fellowship Program[NRF-2015H1D3A1066561, 2019H1D3A1A01102564, 2019R1F1A1059721, 2021R1A6A3A01086420, 2022R1C1C1005255, 2022R1F1A1075115] ; Netherlands Research School for Astronomy (NOVA) Virtual Institute of Accretion (VIA) postdoctoral fellowships ; NOIRLab ; Swedish Research Council[2017-00648] ; Perimeter Institute for Theoretical Physic (Government of Canada through the Department of Innovation, Science and Economic Development) ; Perimeter Institute for Theoretical Physic (Province of Ontario through the Ministry of Research, Innovation and Science) ; Princeton Gravity Initiative ; Spanish Ministerio de Ciencia e Innovacion[PGC2018-098915-B-C21, AYA2016-80889-P, PID2019-108995GB-C21, PID2020-117404GB-C21] ; University of Pretoria ; Shanghai Municipality orientation program of basic research for international scientists[22JC1410600] ; Shanghai Pilot Program for Basic Research, Chinese Academy of Science, Shanghai Branch[JCYJ-SHFY-2021-013] ; State Agency for Research of the Spanish MCIU through the Center of Excellence Severo Ochoa[SEV-2017-0709] ; Spanish Ministry for Science and Innovation - MCIN/AEI[CEX2021-001131-S] ; Spinoza Prize[SPI 78-409] ; South African Research Chairs Initiative, through the South African Radio Astronomy Observatory (SARAO)[77948] ; Toray Science Foundation ; Swedish Research Council (VR) ; UK Science and Technology Facilities Council[ST/X508329/1] ; US Department of Energy (USDOE) through the Los Alamos National Laboratory ; National Nuclear Security Administration of the USDOE[89233218CNA000001] ; YCAA Prize Postdoctoral Fellowship ; Office of Science of the U.S. Department of Energy[DE-AC05-00OR22725] ; ASTROVIVES FEDER infrastructure[IDIFEDER-2021-086] ; Special Fund for Astronomy from the Ministry of Finance in China ; A FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)[2021/01183-8] ; Smithsonian Institution ; A National Key Research and Development Program of China[2017YFA0402700] ; A Natural Science Foundation of China[11873028, 2030508, 1836650] ; Kavli Institute of Cosmological Physics at the University of Chicago ; NSF[ACI-1548562, DBI-0735191 DBI1265383 DBI-1743442] ; Conicyt[QUIMAL170001, PIA ACT172033] ; A Fondecyt[11170268, 220002] ; Compute Ontario ; Calcul Quebec ; Compute Canada
内容类型	期刊论文
版本	出版稿
源URL	[http://ir.ynao.ac.cn/handle/114a53/27149]
专题	云南天文台_中国科学院天体结构与演化重点实验室
作者单位	1.Department of Physics and Astronomy, Michigan State University, 567 Wilson Road, East Lansing, MI 48824, USA 2.Astronomy Department, University of Science and Technology of China, Hefei 230026, People's Republic of China; 3.Center for Astronomy and Astrophysics and Department of Physics, Fudan University, Shanghai 200438, People's Republic of China; 4.Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK; 5.School of Physics, Huazhong University of Science and Technology, Wuhan, Hubei, 430074, People's Republic of China; 6.School of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ 08540, USA; 7.Radboud Excellence Fellow of Radboud University, Nijmegen, The Netherlands; 8.Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Finland; 9.Physics Department, Brandeis University, 415 South Street, Waltham, MA 02453, USA; 10.University of New Mexico, Department of Physics and Astronomy, Albuquerque, NM 87131, USA;
推荐引用方式 GB/T 7714	Akiyama, Kazunori,Alberdi, Antxon,Alef, Walter,et al. First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,964(2).
APA	Akiyama, Kazunori.,Alberdi, Antxon.,Alef, Walter.,Algaba, Juan Carlos.,Anantua, Richard.,...&Najafi-Ziyazi, Mahdi.(2024).First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring.ASTROPHYSICAL JOURNAL LETTERS,964(2).
MLA	Akiyama, Kazunori,et al."First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring".ASTROPHYSICAL JOURNAL LETTERS 964.2(2024).