YNAO OpenIR  > 星系类星体研究组
The putative center in NGC1052
Baczko, Anne-Kathrin1,2; Kadler, Matthias3; Ros, Eduardo2; Fromm, Christian M.2,3,4; Wielgus, Maciek2; Perucho, Manel5,6; Krichbaum, Thomas P.2; Baloković, Mislav7; Blackburn, Lindy8,9; Chan, Chi-kwan10,11,12; Issaoun, Sara9; Janssen, Michael2,13; Ricci, Luca2,3; Akiyama, Kazunori8,14,15; Albentosa, Ezequiel5; Alberdi, Antxon16; Alef, Walter2; Algaba, Juan Carlos17; Anantua, Richard8,9,18,140; Asada, Keiichi19; Azulay, Rebecca2,5,6; Bach, Uwe2; Ball, David10; Bandyopadhyay, Bidisha20; Barrett, John14; Bauböck, Michi21; Benson, Bradford A.22,23; Bintley, Dan24,25; Blundell, Raymond9; Bouman, Katherine L.26; Bower, Geoffrey C.27,28; Boyce, Hope29,30; Bremer, Michael31; Brinkerink, Christiaan D.13; Brissenden, Roger8,9; Britzen, Silke2; Broderick, Avery E.32,33,34; Broguiere, Dominique31; Bronzwaer, Thomas13; Bustamante, Sandra35; Byun, Do-Young36,37; Carlstrom, John E.23,38,39,40; Ceccobello, Chiara41; Chael, Andrew42; Chang, Dominic O.8,9; Chatterjee, Koushik8,9; Chatterjee, Shami43; Chen, Ming-Tang27; Chen, Yongjun44,45; Cheng, Xiaopeng36; Cho, Ilje16,36,46; Christian, Pierre47; Conroy, Nicholas S.9,48; Conway, John E.41; Cordes, James M.43; Crawford, Thomas M.23,38; Crew, Geoffrey B.14; Cruz, Alejandro4,49; Cui, Yuzhu50,51; Dahale, Rohan16; Davelaar, Jordy113; Laurentis, Mariafelicia De4,54,55; Deane, Roger56,57,58; Dempsey, Jessica24,25,59; Desvignes, Gregory2,60; Dexter, Jason61; Dhruv, Vedant21; Dihingia, Indu K.51; Doeleman, Sheperd S.8,9; Dougall, Sean Taylor10; Dzib, Sergio A.2,31; Eatough, Ralph P.2,62; Emami, Razieh9; Falcke, Heino13; Farah, Joseph63,64; Fish, Vincent L.14; Fomalont, Edward65; Ford, H. Alyson10; Foschi, Marianna16; Fraga, Raquel13; Freeman, William T.66,67; Friberg, Per24,25; Fuentes, Antonio16; Galison, Peter8,68,69; Gammie, Charles F.21,48,70; García, Roberto31; Gentaz, Olivier31; Georgiev, Boris10; Goddi, Ciriaco71,72,73,74; Gold, Roman75; Gómez, Arturo I.76,77; Gómez, José L.16; Gu, Minfeng44,78; Gurwell, Mark9; Hada, Kazuhiro79,80; Haggard, Daryl29,30; Haworth, Kari9; Hecht, Michael H.14; Hesper, Ronald81; Heumann, Dirk10; Ho, Luis C.82,83; Ho, Paul19,24,25; Honma, Mareki84,85,86; Huang, Chih-Wei L.19; Huang, Lei44,78; Hughes, David H.76; Impellizzeri, C. M. Violette65,87; Inoue, Makoto19; James, David J.88,89; Jannuzi, Buell T.10; Jeter, Britton19; Jiang, Wu44; Jiménez, Alejandra13; Johnson, Michael D.8,9; Jorstad, Svetlana90; Joshi, Abhishek V.21; Jung, Taehyun36,37; Karami, Mansour32,33; Karuppusamy, Ramesh2; Kawashima, Tomohisa91; Keating, Garrett K.9; Kettenis, Mark92; Kim, Dong-Jin2; Kim, Jae-Young2,93; Kim, Jongsoo36; Kim, Junhan94; Kino, Motoki15,95; Koay, Jun Yi19; Kocherlakota, Prashant4; Kofuji, Yutaro84,86; Koyama, Shoko19,96; Kramer, Carsten31; Kramer, Joana A.2; Kramer, Michael2; Kuo, Cheng-Yu19,97; Bella, Noemi La13; Lauer, Tod R.98; Lee, Daeyoung21; Lee, Sang-Sung36; Leung, Po Kin99; Levis, Aviad26; Li, Zhiyuan100,101; Lico, Rocco16,102; Lindahl, Greg9; Lindqvist, Michael41; Lisakov, Mikhail103; Liu, Jun2; Liu, Kuo2; Liuzzo, Elisabetta104; Lo, Wen-Ping19,105; Lobanov, Andrei P.2; Loinard, Laurent106; Lonsdale, Colin J.14; Lowitz, Amy E.10; Lu, Ru-Sen2,44,107; MacDonald, Nicholas R.2; Mao JR(毛基荣)108,109,110; Marchili, Nicola2,104; Markoff, Sera111,112; Marrone, Daniel P.10; Marscher, Alan P.90; Martí, Iván5,6; Matsushita, Satoki19; Matthews, Lynn D.14; Medeiros, Lia113; Menten, Karl M.2; Michalik, Daniel23,114; Mizuno, Izumi24,25; Mizuno, Yosuke4,51,115; Moran, James M.8,9; Moriyama, Kotaro4,14,84; Moscibrodzka, Monika13; Mulaudzi, Wanga111; Müller, Cornelia2,13; Müller, Hendrik2; Mus, Alejandro72,104; Musoke, Gibwa13,111; Myserlis, Ioannis116; Nadolski, Andrew48; Nagai, Hiroshi15,85; Nagar, Neil M.20; Nair, Dhanya G.20; Nakamura, Masanori19,117; Narayanan, Gopal35; Natarajan, Iniyan8,9; Nathanail, Antonios4,118; Fuentes, Santiago Navarro116; Neilsen, Joey119; Neri, Roberto31; Ni, Chunchong32,33,34; Noutsos, Aristeidis2; Nowak, Michael A.120; Oh, Junghwan92; Okino, Hiroki84,86; Sánchez, Héctor Raúl Olivares121; Ortiz, Gisela N.2,76; Oyama, Tomoaki84; Özel, Feryal122; Palumbo, Daniel C. M.8,9; Paraschos, Georgios Filippos2; Park, Jongho19,123; Parsons, Harriet24,25; Patel, Nimesh9; Pen, Ue-Li19,32,124,125,126; Pesce, Dominic W.8,9; Piétu, Vincent31; Plambeck, Richard127; PopStefanija, Aleksandar35; Porth, Oliver4,111; Pötzl, Felix M.2,128; Prather, Ben21; Preciado, Jorge A.32; Principe, Giacomo102,129,130; Psaltis, Dimitrios122; Pu, Hung-Yi19,131,132; Ramakrishnan, Venkatessh20,133,134; Rao, Ramprasad9; Rawlings, Mark G.24,25,135; Raymond, Alexander W.8,9; Ricarte, Angelo8,9; Ripperda, Bart32,124,125,136; Roelofs, Freek8,9,13; Rogers, Alan14; Romero, Cristina19; Roshanineshat, Arash10; Rottmann, Helge2; Roy, Alan L.2; Ruiz, Ignacio116; Ruszczyk, Chet14; Rygl, Kazi L. J.104; Sánchez, Salvador116; Sánchez, David76,77; Sánchez, Miguel116; Sasada, Mahito84,137,138; Satapathy, Kaushik10; Savolainen, Tuomas2,134,139; Schloerb, F. Peter35; Schonfeld, Jonathan9; Schuster, Karl-Friedrich31; Shao, Lijing2,83; Shen, Zhiqiang44,45; Small, Des92; Sohn, Bong Won36,37,46; SooHoo, Jason16; Salas, León David Sosapanta111; Souccar, Kamal35; Stanway, Joshua S.141; Sun, He142,143; Tazaki, Fumie84; Tetarenko, Alexandra J.144; Tiede, Paul8,9; Tilanus, Remo P. J.10,13,87,145; Titus, Michael14; Torne, Pablo2,116; Toscano, Teresa16; Traianou, Efthalia2,16; Trent, Tyler10; Trippe, Sascha146; Turk, Matthew48; Bemmel, Ilse van92; Langevelde, Huib Jan van87,92,147; Rossum, Daniel R. van13; Vos, Jesse13; Wagner, Jan2; Ward, Derek141; Wardle, John148; Washington, Jasmin E.10; Weintroub, Jonathan8,9; Wharton, Robert2; Wiik, Kaj149; Witzel, Gunther2; Wondrak, Michael F.13,150; Wong, George N.42,151; Wu, Qingwen152; Yadlapalli, Nitika26; Yamaguchi, Paul9; Yfantis, Aristomenis13; Yoon, Doosoo111; Young, André13; Young, Ken9; Younsi, Ziri4,153; Yu, Wei9; Yuan, Feng154; Yuan, Ye-Fei155; Zensus, J. Anton2; Zhang, Shuo156; Zhao, Guang-Yao2,16
发表期刊ASTRONOMY & ASTROPHYSICS (IF:5.565[JCR-2017],4.902[5-Year])
2024-12-17
卷号692
DOI10.1051/0004-6361/202450898
产权排序第109完成单位
收录类别SCI ; EI
摘要Context. Many active galaxies harbor powerful relativistic jets, however, the detailed mechanisms of their formation and acceleration remain poorly understood. Aims. To investigate the area of jet acceleration and collimation with the highest available angular resolution, we study the innermost region of the bipolar jet in the nearby low-ionization nuclear emission-line region (LINER) galaxy NGC1052. Methods. We combined observations of NGC1052 taken with VLBA, GMVA, and EHT over one week in the spring of 2017. Our study is focused on the size and continuum spectrum of the innermost region containing the central engine and the footpoints of both jets. We employed a synchrotron-self absorption model to fit the continuum radio spectrum and we combined the size measurements from close to the central engine out to similar to 1 pc to study the jet collimation. Results. For the first time, NGC1052 was detected with the EHT, providing a size of the central region in-between both jet bases of 43 mu as perpendicular to the jet axes, corresponding to just around 250 R-S (Schwarzschild radii). This size estimate supports previous studies of the jets expansion profile which suggest two breaks of the profile at around 3 x 10(3) R-S and 1 similar to 10(4) R-S distances to the core. Furthermore, we estimated the magnetic field to be 1.25 Gauss at a distance of 22 mu as from the central engine by fitting a synchrotron-self absorption spectrum to the innermost emission feature, which shows a spectral turn-over at similar to 130 GHz. Assuming a purely poloidal magnetic field, this implies an upper limit on the magnetic field strength at the event horizon of 2:6 x 10(4) Gauss, which is consistent with previous measurements. Conclusions. The complex, low-brightness, double-sided jet structure in NGC1052 makes it a challenge to detect the source at millimeter (mm) wavelengths. However, our first EHT observations have demonstrated that detection is possible up to at least 230 GHz. This study o ffers a glimpse through the dense surrounding torus and into the innermost central region, where the jets are formed. This has enabled us to finally resolve this region and provide improved constraints on its expansion and magnetic field strength.
资助项目international Gemini Observatory; NSF NOIRLab; U.S. National Science Foundation; United States of America; National Research Foundation of Korea(NRF) - Korea government(MSIT)[RS-2024-00449206]; NASA through the NASA Hubble Fellowship[HST-HF2-51552.001A]; Space Telescope Science Institute; NASA[NAS5-26555]
项目资助者international Gemini Observatory ; NSF NOIRLab ; U.S. National Science Foundation ; United States of America ; National Research Foundation of Korea(NRF) - Korea government(MSIT)[RS-2024-00449206] ; NASA through the NASA Hubble Fellowship[HST-HF2-51552.001A] ; Space Telescope Science Institute ; NASA[NAS5-26555]
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
文章类型Article
出版者EDP SCIENCES S A
出版地17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
ISSN0004-6361
URL查看原文
WOS记录号WOS:001410383100001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]ACTIVE GALACTIC NUCLEI ; LOW-LUMINOSITY AGN ; NGC 1052 ; H2O MASER ; JET ; RADIO ; ACCRETION ; TORUS ; NGC-1052 ; FLOWS
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文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/28172
专题星系类星体研究组
中国科学院天体结构与演化重点实验室
作者单位1.Department of Space, Earth and Environment, Chalmers University of Technology, SE-41296 Gothenburg, Sweden;
2.Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany;
3.Institut für Theoretische Physik und Astrophysik, Universität Würzburg, Emil-Fischer-Str. 31, D-97074 Würzburg, Germany;
4.Institut für Theoretische Physik, Goethe-Universität Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt am Main, Germany;
5.Departament d’Astronomia i Astrofísica, Universitat de València, C. Dr. Moliner 50, E-46100 Burjassot, València, Spain;
6.Observatori Astronòmic, Universitat de València, C. Catedrático José Beltrán 2, E-46980 Paterna, València, Spain;
7.Yale Center for Astronomy & Astrophysics, Yale University, 52 Hillhouse Avenue, New Haven, CT 06511, USA;
8.Black Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USA;
9.Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA;
10.Steward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA;
11.Data Science Institute, University of Arizona, 1230 N. Cherry Ave., Tucson, AZ 85721, USA;
12.Program in Applied Mathematics, University of Arizona, 617 N. Santa Rita, Tucson, AZ 85721, USA;
13.Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, PO Box 9010 6500 GL Nijmegen, The Netherlands;
14.Massachusetts Institute of Technology Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USA;
15.National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
16.Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, Spain;
17.Department of Physics, Faculty of Science, Universiti Malaya, 50603 Kuala Lumpur, Malaysia;
18.Department of Physics & Astronomy, The University of Texas at San Antonio, One UTSA Circle, San Antonio, TX 78249, USA;
19.Institute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Sec. 4, Roosevelt Rd., Taipei 10617, Taiwan, ROC;
20.Astronomy Department, Universidad de Concepción, Casilla 160-C Concepción, Chile;
21.Department of Physics, University of Illinois, 1110 West Green Street, Urbana, IL 61801, USA;
22.Fermi National Accelerator Laboratory, MS209, PO Box 500 Batavia, IL 60510, USA;
23.Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA;
24.East Asian Observatory, 660 N. A’ohoku Place, Hilo, HI 96720, USA;
25.James Clerk Maxwell Telescope (JCMT), 660 N. A’ohoku Place, Hilo, HI 96720, USA;
26.California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA;
27.Institute of Astronomy and Astrophysics, Academia Sinica, 645 N. A’ohoku Place, Hilo, HI 96720, USA;
28.Department of Physics and Astronomy, University of Hawaii at Manoa, 2505 Correa Road, Honolulu, HI 96822, USA;
29.Department of Physics, McGill University, 3600 rue University, Montréal, QC H3A 2T8, Canada;
30.Trottier Space Institute at McGill, 3550 rue University, Montréal, QC H3A 2A7, Canada;
31.Institut de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, F-38406 Saint Martin d’Hères, France;
32.Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, ON N2L 2Y5, Canada;
33.Department of Physics and Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, ON N2L 3G1, Canada;
34.Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1, Canada;
35.Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA;
36.Korea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of Korea;
37.University of Science and Technology, Gajeong-ro 217, Yuseong-gu, Daejeon 34113, Republic of Korea;
38.Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA;
39.Department of Physics, University of Chicago, 5720 South Ellis Avenue, Chicago, IL 60637, USA;
40.Enrico Fermi Institute, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA;
41.Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala, Sweden;
42.Princeton Gravity Initiative, Jadwin Hall, Princeton University, Princeton, NJ 08544, USA;
43.Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USA;
44.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, PR China;
45.Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100101, PR China;
46.Department of Astronomy, Yonsei University, Yonsei-ro 50, Seodaemun-gu, 03722 Seoul, Republic of Korea;
47.Physics Department, Fairfield University, 1073 North Benson Road, Fairfield, CT 06824, USA;
48.Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801, USA;
49.Instituto de Astronomía, Universidad Nacional Autónoma de México (UNAM), Apdo Postal 70-264, Ciudad de México, Mexico;
50.Research Center for Astronomical Computing, Zhejiang Laboratory, Hangzhou 311100, PR China;
51.Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shengrong Road 520, Shanghai 201210, PR China;
52.Department of Astronomy and Columbia Astrophysics Laboratory, Columbia University, 500 W. 120th Street, New York, NY 10027, USA;
53.Center for Computational Astrophysics, Flatiron Institute, 162 Fifth Avenue, New York, NY 10010, USA;
54.Dipartimento di Fisica “E. Pancini”, Università di Napoli “Federico II”, Compl. Univ. di Monte S. Angelo, Edificio G, Via Cinthia, I-80126 Napoli, Italy;
55.INFN Sez. di Napoli, Compl. Univ. di Monte S. Angelo, Edificio G, Via Cinthia, I-80126 Napoli, Italy;
56.Wits Centre for Astrophysics, University of the Witwatersrand, 1 Jan Smuts Avenue, Braamfontein, Johannesburg 2050, South Africa;
57.Department of Physics, University of Pretoria, Hatfield, Pretoria 0028, South Africa;
58.Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Makhanda 6140, South Africa;
59.ASTRON, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands;
60.LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, F-92195 Meudon, France;
61.JILA and Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO 80309, USA;
62.National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100101, PR China;
63.Las Cumbres Observatory, 6740 Cortona Drive, Suite 102, Goleta, CA 93117-5575, USA;
64.Department of Physics, University of California, Santa Barbara, CA 93106-9530, USA;
65.National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, USA;
66.Department of Electrical Engineering and Computer Science, Massachusetts Institute of Technology, 32-D476, 77 Massachusetts Ave., Cambridge, MA 02142, USA;
67.Google Research, 355 Main St., Cambridge, MA 02142, USA;
68.Department of History of Science, Harvard University, Cambridge, MA 02138, USA;
69.Department of Physics, Harvard University, Cambridge, MA 02138, USA;
70.NCSA, University of Illinois, 1205 W. Clark St., Urbana, IL 61801, USA;
71.Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, R. do Matão, 1226, São Paulo, SP 05508-090, Brazil;
72.Dipartimento di Fisica, Universitá degli Studi di Cagliari, SP Monserrato-Sestu km 0.7, I-09042 Monserrato, Italy;
73.INAF – Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (CA), Italy;
74.INFN, sezione di Cagliari, I-09042 Monserrato, (CA), Italy;
75.CP3-Origins, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark;
76.Instituto Nacional de Astrofísica, Óptica y Electrónica, Apartado Postal 51 y 216, 72000 Puebla Pue., Mexico;
77.Consejo Nacional de Humanidades, Ciencia y Tecnología, Av. Insurgentes Sur 1582, 03940 Ciudad de México, Mexico;
78.Key Laboratory for Research in Galaxies and Cosmology, Chinese Academy of Sciences, Shanghai 200030, PR China;
79.Graduate School of Science, Nagoya City University, Yamanohata 1, Mizuho-cho, Mizuho-ku, Nagoya, 467-8501 Aichi, Japan;
80.Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka-cho, Mizusawa, Oshu, 023-0861 Iwate, Japan;
81.NOVA Sub-mm Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The Netherlands;
82.Department of Astronomy, School of Physics, Peking University, Beijing 100871, PR China;
83.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, PR China;
84.Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-12 Hoshigaoka, Mizusawa, Oshu, Iwate 023-0861, Japan;
85.Department of Astronomical Science, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
86.Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan;
87.Leiden Observatory, Leiden University, Postbus 2300, 9513 RA Leiden, The Netherlands;
88.ASTRAVEO LLC, PO Box 1668 Gloucester, MA 01931, USA;
89.Applied Materials Inc., 35 Dory Road, Gloucester, MA 01930, USA;
90.Institute for Astrophysical Research, Boston University, 725 Commonwealth Ave., Boston, MA 02215, USA;
91.Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8582, Japan;
92.Joint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands;
93.Department of Physics, Ulsan National Institute of Science and Technology (UNIST), 50 UNIST-gil, Eonyang-eup, Ulju-gun, Ulsan 44919, Republic of Korea;
94.Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), 291 Daehak-ro, Yuseong-gu, Daejeon 34141, Republic of Korea;
95.Kogakuin University of Technology & Engineering, Academic Support Center, 2665-1 Nakano, Hachioji, Tokyo 192-0015, Japan;
96.Graduate School of Science and Technology, Niigata University, 8050 Ikarashi 2-no-cho, Nishi-ku, Niigata 950-2181, Japan;
97.Physics Department, National Sun Yat-Sen University, No. 70, Lien-Hai Road, Kaosiung City 80424, Taiwan, ROC;
98.National Optical Astronomy Observatory, 950 N. Cherry Ave., Tucson, AZ 85719, USA;
99.Department of Physics, The Chinese University of Hong Kong, Shatin, N. T., Hong Kong;
100.School of Astronomy and Space Science, Nanjing University, Nanjing 210023, PR China;
101.Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing 210023, PR China;
102.INAF-Istituto di Radioastronomia, Via P. Gobetti 101, I-40129 Bologna, Italy;
103.Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla, 4059 Valparaíso, Chile;
104.INAF-Istituto di Radioastronomia & Italian ALMA Regional Centre, Via P. Gobetti 101, I-40129 Bologna, Italy;
105.Department of Physics, National Taiwan University, No. 1, Sec. 4, Roosevelt Rd., Taipei 10617, Taiwan, ROC;
106.Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, Mexico;
107.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, PR China;
108.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, Yunnan Province, PR China;
109.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, PR China;
110.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, PR China;
111.Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands;
112.Gravitation and Astroparticle Physics Amsterdam (GRAPPA) Institute, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands;
113.Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA;
114.Science Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1 2201 AZ Noordwijk, The Netherlands;
115.School of Physics and Astronomy, Shanghai Jiao Tong University, 800 Dongchuan Road, Shanghai 200240, PR China;
116.Institut de Radioastronomie Millimétrique (IRAM), Avenida Divina Pastora 7, Local 20, E-18012 Granada, Spain;
117.National Institute of Technology, Hachinohe College, 16-1 Uwanotai, Tamonoki, Hachinohe City, Aomori 039-1192, Japan;
118.Research Center for Astronomy, Academy of Athens, Soranou Efessiou 4, 115 27 Athens, Greece;
119.Department of Physics, Villanova University, 800 Lancaster Avenue, Villanova, PA 19085, USA;
120.Physics Department, Washington University, CB 1105, St. Louis, MO 63130, USA;
121.Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications (CIDMA), Campus de Santiago, 3810-193 Aveiro, Portugal;
122.School of Physics, Georgia Institute of Technology, 837 State St NW, Atlanta, GA 30332, USA;
123.School of Space Research, Kyung Hee University, 1732, Deogyeong-daero, Giheung-gu, Yongin-si, Gyeonggi-do 17104, Republic of Korea;
124.Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada;
125.Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4, Canada;
126.Canadian Institute for Advanced Research, 180 Dundas St West, Toronto, ON M5G 1Z8, Canada;
127.Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA;
128.Institute of Astrophysics, Foundation for Research and Technology – Hellas, Voutes, 7110 Heraklion, Greece;
129.Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy;
130.INFN Sez. di Trieste, I-34127 Trieste, Italy;
131.Department of Physics, National Taiwan Normal University, No. 88, Sec. 4, Tingzhou Rd., Taipei 116, Taiwan, ROC;
132.Center of Astronomy and Gravitation, National Taiwan Normal University, No. 88, Sec. 4, Tingzhou Road, Taipei 116, Taiwan, ROC;
133.Finnish Centre for Astronomy with ESO, FI-20014 University of Turku, Finland;
134.Aalto University Metsähovi Radio Observatory, Metsähovintie 114, FI-02540 Kylmälä, Finland;
135.Gemini Observatory/NSF’s NOIRLab, 670 N. A’ohōkū Place, Hilo, HI 96720, USA;
136.Department of Physics, University of Toronto, 60 St. George Street, Toronto, ON M5S 1A7, Canada;
137.Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan;
138.Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan;
139.Aalto University Department of Electronics and Nanoengineering, PL 15500, FI-00076 Aalto, Finland;
140.Physics & Astronomy Department, Rice University, Houston, Texas 77005-1827, USA;
141.Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK;
142.National Biomedical Imaging Center, Peking University, Beijing 100871, PR China;
143.College of Future Technology, Peking University, Beijing 100871, PR China;
144.Department of Physics and Astronomy, University of Lethbridge, Lethbridge, Alberta T1K 3M4, Canada;
145.Netherlands Organisation for Scientific Research (NWO), Postbus 93138, 2509 AC Den Haag, The Netherlands;
146.Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul 08826, Republic of Korea;
147.University of New Mexico, Department of Physics and Astronomy, Albuquerque, NM 87131, USA;
148.Physics Department, Brandeis University, 415 South Street, Waltham, MA 02453, USA;
149.Tuorla Observatory, Department of Physics and Astronomy, University of Turku, FI-20014 TURUN YLIOPISTO, Finland;
150.Radboud Excellence Fellow of Radboud University, Nijmegen, The Netherlands;
151.School of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ 08540, USA;
152.School of Physics, Huazhong University of Science and Technology, Wuhan, Hubei 430074, PR China;
153.Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK;
154.Center for Astronomy and Astrophysics and Department of Physics, Fudan University, Shanghai 200438, PR China;
155.Astronomy Department, University of Science and Technology of China, Hefei 230026, PR China;
156.Department of Physics and Astronomy, Michigan State University, 567 Wilson Rd, East Lansing, MI 48824, USA
推荐引用方式
GB/T 7714
Baczko, Anne-Kathrin,Kadler, Matthias,Ros, Eduardo,et al. The putative center in NGC1052[J]. ASTRONOMY & ASTROPHYSICS,2024,692.
APA Baczko, Anne-Kathrin.,Kadler, Matthias.,Ros, Eduardo.,Fromm, Christian M..,Wielgus, Maciek.,...&Zhao, Guang-Yao.(2024).The putative center in NGC1052.ASTRONOMY & ASTROPHYSICS,692.
MLA Baczko, Anne-Kathrin,et al."The putative center in NGC1052".ASTRONOMY & ASTROPHYSICS 692(2024).
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