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Ordered magnetic fields around the 3C 84 central black hole

文献类型：期刊论文

作者Paraschos, G. F.153; Kim, J.-Y.152,153; Wielgus, M.151,153; Röder, J.153; Krichbaum, T. P.153; Ros, E.153; Agudo, I.150; Myserlis, I.149,153; Moscibrodzka, M.148; Traianou, E.150,153
刊名ASTRONOMY & ASTROPHYSICS
出版日期2024-02-01
卷号682
ISSN号0004-6361
关键词techniques: high angular resolution techniques: interferometric galaxies: active galaxies: individual: NGC 1275 galaxies: jets
DOI10.1051/0004-6361/202348308
产权排序第107完成单位
文献子类Article
英文摘要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 gamma(m) = (113 +/- 4) GHz, a corresponding synchrotron self-absorbed magnetic field of B-SSA = (2.9 +/- 1.6) G, and an equipartition magnetic field of B-eq = (5.2 +/- 0.6) G. Three components are resolved with the highest fractional polarisation detected for this object (m(net) = (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 di fferent 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 o ffer full imaging capabilities, will shed more light on the compact region of 3C 84.
学科主题天文学 ; 星系与宇宙学
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出版地17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
WOS关键词M87 EVENT HORIZON ; EXTRAGALACTIC RADIO-SOURCES ; TELESCOPE RESULTS. I. ; LIMB-BRIGHTENED JET ; GAMMA-RAY EMISSION ; LINEAR-POLARIZATION ; ACCRETION ; PARSEC ; ENERGY ; SCALE
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]; Alexander von Humboldt Stiftung; Alfred P. Sloan Research Fellowship; Allegro, the European ALMA Regional Centre node in the Netherlands; NL astronomy research network NOVA; ALMA North America Development Fund; Astrophysics and High Energy Physics programme by MCIN (European Union NextGenerationEU)[PRTR-C17I1]; University of Amsterdam; Black Hole Initiative - John Templeton Foundation; Gordon and Betty Moore Foundation; Brinson Foundation; la Caixa Foundation[100010434]; la Caixa Foundation[LCF/BQ/DI22/11940027]; la Caixa Foundation[LCF/BQ/DI22/11940030]; la Caixa Foundation[Chandra DD7-18089X]; la Caixa Foundation[TM6-17006X]; China Scholarship Council; China Postdoctoral Science Foundation[2020M671266]; China Postdoctoral Science Foundation[2022M712084]; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[U0004-246083]; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[U0004-259839]; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[F0003-272050]; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[F0003-281692]; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[104497]; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[275201]; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[263356]; 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)[IN112417]; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN112820]; Dutch Black Hole Consortium of the research programme the National Science Agenda[NWA 1292.19.202]; Dutch Organization for Scientific Research (NWO)[639.043.513]; Dutch Organization for Scientific Research (NWO)[OCENW.KLEIN.113]; Dutch National Supercomputers, Cartesius and Snellius (NWO grant)[2021.013]; EACOA Fellowship - East Asia Core Observatories Association, Academia Sinica Institute of Astronomy and Astrophysics,; Korea Astronomy and Space Science Institute; European Research Council (ERC) Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058]; European Union[730562]; European Union[101018682]; Horizon ERC[101040021]; Generalitat Valenciana[APOSTD/2018/177]; Generalitat Valenciana[ASFAE/2022/018]; Generalitat Valenciana[CIDE-GENT/2018/021]; MICINN Research Project[PID2019-108995GB-C22]; European Research Council[884631]; FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)[2021/01183-8]; Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEONGRAV; DFG research grant Jet physics on horizon scales and beyond[FR 4069/2-1]; Joint Columbia/Flatiron Postdoctoral Fellowship (Simons Foundation); Leiden University; 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)[QYZDJSSW-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; 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]; Malaysian Fundamental Research Grant Scheme (FRGS)[FRGS/1/2019/STG02/UM/02/6]; 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-001017]; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-020]; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-041]; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-110-005]; Ministry of Science and Technology (MOST) of Taiwan[107-2923-M-001-009]; Ministry of Science and Technology (MOST) of Taiwan[108-2112-M-001-048]; Ministry of Science and Technology (MOST) of Taiwan[108-2112-M-001-051]; Ministry of Science and Technology (MOST) of Taiwan[108-2923-M-001-002]; Ministry of Science and Technology (MOST) of Taiwan[109-2112-M-001-025]; Ministry of Science and Technology (MOST) of Taiwan[109-2124-M-001-005]; Ministry of Science and Technology (MOST) of Taiwan[109-2923-M-001-001]; Ministry of Science and Technology (MOST) of Taiwan[110-2112-M-003-007-MY2]; Ministry of Science and Technology (MOST) of Taiwan[110-2112-M-001-033]; Ministry of Science and Technology (MOST) of Taiwan[110-2124-M-001-007]; Ministry of Science and Technology (MOST) of Taiwan[110-2923-M-001-001]; Ministry of Education (MoE) of Taiwan Yushan Young Scholar Program; National Aeronautics and Space Administration (NASA)[80NSSC20K1567]; National Aeronautics and Space Administration (NASA)[80NSSC20K0527]; National Aeronautics and Space Administration (NASA)[80NSSC20K0645]; NASA Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51431.001-A]; NASA Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51482.001-A]; NASA Hubble Fellowship - Space Telescope Science Institute[NAS5-26555]; 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 Key Research and Development Program of China[2017YFA0402700]; National Science Foundation (NSF)[AST-0096454]; National Science Foundation (NSF)[AST-0352953]; National Science Foundation (NSF)[AST-0521233]; National Science Foundation (NSF)[AST-0705062]; National Science Foundation (NSF)[AST-0905844]; National Science Foundation (NSF)[AST-0922984]; National Science Foundation (NSF)[AST-1126433]; National Science Foundation (NSF)[DGE-1144085]; National Science Foundation (NSF)[AST-1207704]; National Science Foundation (NSF)[AST-1207752]; National Science Foundation (NSF)[MRI-1228509]; 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 Sciences and Engineering Research Council of Canada (NSERC); National Youth Thousand Talents Program of China; National Research Foundation of Korea[NRF-2015H1A2A1033752]; National Research Foundation of Korea[NRF-2015H1D3A1066561]; National Research Foundation of Korea[2019H1D3A1A01102564]; National Research Foundation of Korea[2019R1F1A1059721]; National Research Foundation of Korea[2021R1A6A3A01086420]; National Research Foundation of Korea[2022R1C1C1005255]; Perimeter Institute for Theoretical Physics (Government of Canada through the Department of Innovation, Science and Economic Development); Perimeter Institute for Theoretical Physics (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; South African Research Chairs Initiative, through the South African Radio Astronomy Observatory (SARAO)[77948]; Toray Science Foundation; Swedish Research Council (VR); US Department of Energy (USDOE) through the Los Alamos National Laboratory; National Nuclear Security Administration of the USDOE[89233218CNA000001]; YCAA Prize Postdoctoral Fellowship; CAS; Radboud University; 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; Smithsonian Institution; Science and Technologies Facility Council (UK); CNRS (Centre National de la Recherche Scientifique, France); MPG (Max-Planck-Gesellschaft, Germany); IGN (Instituto Geografico Nacional, Spain); State of Arizona; Kavli Institute of Cosmological Physics at the University of Chicago; National Science Foundation[OPP-1852617]; National Science Foundation[ACI-1548562]; National Science Foundation[DBI-0735191]; National Science Foundation[DBI-1265383]; National Science Foundation[DBI-1743442]; National Science Foundation[OAC-1818253]; National Science Foundation[2030508]; National Science Foundation[1836650]; Frontera computing project at the Texas Advanced Computing Center through the Frontera Large-Scale Community Partnerships[AST20023]; Compute Ontario; Calcul Quebec; Compute Canada; National Astronomical Observatory of Japan; Center for Astronomical Mega-Science, Chinese Academy of Sciences; Institute for Advanced Study; International Max Planck Research School for Astronomy and Astrophysics at the University of Bonn; International Max Planck Research School for Astronomy and Astrophysics at the University of Cologne; Physics Division, National Center for Theoretical Sciences of Taiwan; National Institute of Natural Sciences (NINS) of Japan; Netherlands Research School for Astronomy (NOVA) Virtual Institute of Accretion (VIA) postdoctoral fellowships; Swedish Research Council[2017-00648]; 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 award[SEV-2017-0709]; Spanish Ministry for Science and Innovation grant - MCIN/AEI[CEX2021-001131-S]; Spinoza Prize[SPI 78-409]; 'National Science Foundation'[OPP-1852617]; 'National Science Foundation'[OPP-1248097]; 'National Science Foundation'[AST-1440254]; 'National Science Foundation'[AST-1555365]; 'National Science Foundation'[AST-1614868]; 'National Science Foundation'[AST-1615796]; 'National Science Foundation'[AST-1715061]; 'National Science Foundation'[AST-1716327]; 'National Science Foundation'[AST-1716536]; 'National Science Foundation'[OISE-1743747]; 'National Science Foundation'[AST-1816420]; 'National Science Foundation'[AST-1935980]; 'National Science Foundation'[AST-2034306]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者EDP SCIENCES S A
WOS记录号WOS:001187956400001
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] ; Alexander von Humboldt Stiftung ; Alfred P. Sloan Research Fellowship ; Allegro, the European ALMA Regional Centre node in the Netherlands ; NL astronomy research network NOVA ; ALMA North America Development Fund ; Astrophysics and High Energy Physics programme by MCIN (European Union NextGenerationEU)[PRTR-C17I1] ; University of Amsterdam ; Black Hole Initiative - John Templeton Foundation ; Gordon and Betty Moore Foundation ; Brinson Foundation ; la Caixa Foundation[100010434, LCF/BQ/DI22/11940027, LCF/BQ/DI22/11940030, Chandra DD7-18089X, TM6-17006X] ; China Scholarship Council ; China Postdoctoral Science Foundation[2020M671266, 2022M712084] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[U0004-246083, U0004-259839, F0003-272050, F0003-281692, 104497, 275201, 263356] ; 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)[IN112417, IN112820] ; Dutch Black Hole Consortium of the research programme the National Science Agenda[NWA 1292.19.202] ; Dutch Organization for Scientific Research (NWO)[639.043.513, OCENW.KLEIN.113] ; Dutch National Supercomputers, Cartesius and Snellius (NWO grant)[2021.013] ; EACOA Fellowship - East Asia Core Observatories Association, Academia Sinica Institute of Astronomy and Astrophysics, ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) Synergy Grant BlackHoleCam: Imaging the Event Horizon of Black Holes[610058] ; European Union[730562, 101018682] ; Horizon ERC[101040021] ; Generalitat Valenciana[APOSTD/2018/177, ASFAE/2022/018, CIDE-GENT/2018/021] ; MICINN Research Project[PID2019-108995GB-C22] ; European Research Council[884631] ; FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo)[2021/01183-8] ; Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEONGRAV ; DFG research grant Jet physics on horizon scales and beyond[FR 4069/2-1] ; Joint Columbia/Flatiron Postdoctoral Fellowship (Simons Foundation) ; Leiden University ; 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, QYZDJSSW-SYS008, ZDBS-LY-SLH011] ; Leverhulme Trust Early Career Research Fellowship ; Max-Planck-Gesellschaft (MPG) ; Max Planck Partner Group of the MPG ; MEXT/JSPS KAKENHI[18KK0090, JP21H01137, JP18H03721, JP18K13594, 18K03709, JP19K14761, 18H01245, 25120007] ; Malaysian Fundamental Research Grant Scheme (FRGS)[FRGS/1/2019/STG02/UM/02/6] ; 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-001017, 107-2119-M-001-020, 107-2119-M-001-041, 107-2119-M-110-005, 107-2923-M-001-009, 108-2112-M-001-048, 108-2112-M-001-051, 108-2923-M-001-002, 109-2112-M-001-025, 109-2124-M-001-005, 109-2923-M-001-001, 110-2112-M-003-007-MY2, 110-2112-M-001-033, 110-2124-M-001-007, 110-2923-M-001-001] ; Ministry of Education (MoE) of Taiwan Yushan Young Scholar Program ; National Aeronautics and Space Administration (NASA)[80NSSC20K1567, 80NSSC20K0527, 80NSSC20K0645] ; NASA Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51431.001-A, HST-HF2-51482.001-A, NAS5-26555] ; National Key Research and Development Program of China[2016YFA0400704, 2017YFA0402703, 2016YFA0400702, 2017YFA0402700] ; National Science Foundation (NSF)[AST-0096454, AST-0352953, AST-0521233, AST-0705062, AST-0905844, AST-0922984, AST-1126433, DGE-1144085, AST-1207704, AST-1207752, MRI-1228509] ; NSF Astronomy and Astrophysics Postdoctoral Fellowship[AST-1903847] ; Natural Science Foundation of China[11650110427, 10625314, 11721303, 11725312, 11873028, 11933007, 11991052, 11991053, 12192220, 12192223] ; Natural Sciences and Engineering Research Council of Canada (NSERC) ; National Youth Thousand Talents Program of China ; National Research Foundation of Korea[NRF-2015H1A2A1033752, NRF-2015H1D3A1066561, 2019H1D3A1A01102564, 2019R1F1A1059721, 2021R1A6A3A01086420, 2022R1C1C1005255] ; Perimeter Institute for Theoretical Physics (Government of Canada through the Department of Innovation, Science and Economic Development) ; Perimeter Institute for Theoretical Physics (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 ; South African Research Chairs Initiative, through the South African Radio Astronomy Observatory (SARAO)[77948] ; Toray Science Foundation ; Swedish Research Council (VR) ; US Department of Energy (USDOE) through the Los Alamos National Laboratory ; National Nuclear Security Administration of the USDOE[89233218CNA000001] ; YCAA Prize Postdoctoral Fellowship ; CAS ; Radboud University ; 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 ; Smithsonian Institution ; Science and Technologies Facility Council (UK) ; CNRS (Centre National de la Recherche Scientifique, France) ; MPG (Max-Planck-Gesellschaft, Germany) ; IGN (Instituto Geografico Nacional, Spain) ; State of Arizona ; Kavli Institute of Cosmological Physics at the University of Chicago ; National Science Foundation[OPP-1852617, ACI-1548562, DBI-0735191, DBI-1265383, DBI-1743442, OAC-1818253, 2030508, 1836650] ; Frontera computing project at the Texas Advanced Computing Center through the Frontera Large-Scale Community Partnerships[AST20023] ; Compute Ontario ; Calcul Quebec ; Compute Canada ; National Astronomical Observatory of Japan ; Center for Astronomical Mega-Science, Chinese Academy of Sciences ; Institute for Advanced Study ; International Max Planck Research School for Astronomy and Astrophysics at the University of Bonn ; International Max Planck Research School for Astronomy and Astrophysics at the University of Cologne ; Physics Division, National Center for Theoretical Sciences of Taiwan ; National Institute of Natural Sciences (NINS) of Japan ; Netherlands Research School for Astronomy (NOVA) Virtual Institute of Accretion (VIA) postdoctoral fellowships ; Swedish Research Council[2017-00648] ; 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 award[SEV-2017-0709] ; Spanish Ministry for Science and Innovation grant - MCIN/AEI[CEX2021-001131-S] ; Spinoza Prize[SPI 78-409] ; 'National Science Foundation'[OPP-1852617, OPP-1248097, AST-1440254, AST-1555365, AST-1614868, AST-1615796, AST-1715061, AST-1716327, AST-1716536, OISE-1743747, AST-1816420, AST-1935980, AST-2034306]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27041]  
专题星系类星体研究组
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 Rd, East Lansing, MI 48824, USA
2.Astronomy Department, University of Science and Technology of China, Hefei 230026, PR China;
3.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, PR 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, PR 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, Turku, Finland;
9.Physics Department, Brandeis University, 415 South Street, Waltham, MA 02453, USA;
10.Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK;
推荐引用方式
GB/T 7714		 Paraschos, G. F.,Kim, J.-Y.,Wielgus, M.,et al. Ordered magnetic fields around the 3C 84 central black hole[J]. ASTRONOMY & ASTROPHYSICS,2024,682.
APA Paraschos, G. F..,Kim, J.-Y..,Wielgus, M..,Röder, J..,Krichbaum, T. P..,...&Zhao, S.-S..(2024).Ordered magnetic fields around the 3C 84 central black hole.ASTRONOMY & ASTROPHYSICS,682.
MLA Paraschos, G. F.,et al."Ordered magnetic fields around the 3C 84 central black hole".ASTRONOMY & ASTROPHYSICS 682(2024).

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