| Title | First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring |
| Authors | Akiyama, Kazunori Alberdi, Antxon Alef, Walter Asada, Keiichi Azulay, Rebecca Baczko, Anne-Kathrin Ball, David Balokovic, Mislav Barrett, John Bintley, Dan Blackburn, Lindy Boland, Wilfred Bouman, Katherine L. Bower, Geoffrey C. Bremer, Michael Brinkerink, Christiaan D. Brissenden, Roger Britzen, Silke Broderick, Avery E. Broguiere, Dominique Bronzwaer, Thomas Byun, Do-Young Carlstrom, John E. Chael, Andrew Chan, Chi-kwan Chatterjee, Shami Chatterjee, Koushik Chen, Ming-Tang Chen, Yongjun Cho, Ilje Christian, Pierre Conway, John E. Cordes, James M. Crew, Geoffrey B. Cui, Yuzhu Davelaar, Jordy De Laurentis, Mariafelicia Deane, Roger Dempsey, Jessica Desvignes, Gregory Dexter, Jason Doeleman, Sheperd S. Eatough, Ralph P. Falcke, Heino Fish, Vincent L. Fomalont, Ed Fraga-Encinas, Raquel Friberg, Per Fromm, Christian M. Gomez, Jose L. Galisonl, Peter Gammie, Charles F. Garcia, Roberto Gentaz, Olivier Georgiev, Boris Goddi, Ciriaco Gold, Roman Gu, Minfeng Gurwell, Mark Hada, Kazuhiro Hecht, Michael H. Hesper, Ronald Ho, Luis C. Ho, Paul Honma, Mareki Huang, Chih-Wei L. Huang, Lei Hughes, David H. Ikeda, Shiro Inoue, Makoto Issaoun, Sara James, David J. Jannuzi, Buell T. Janssen, Michael Jeter, Britton Jiang, Wu Johnson, Michael D. Jorstad, Svetlana Jung, Taehyun Karami, Mansour Karuppusamy, Ramesh Kawashima, Tomohisa Keating, Garrett K. Kettenis, Mark Kim, Jae-Young Kim, Junhan Kim, Jongsoo Kino, Motoki Koay, Jun Yi Koch, Patrick M. Koyama, Shoko Kramer, Michael Kramer, Carsten Krichbaum, Thomas P. Kuo, Cheng-Yu Lauer, Tod R. Lee, Sang-Sung Li, Yan-Rong Li, Zhiyuan Lindqvist, Michael Liu, Kuo Liuzzo, Elisabetta Lo, Wen-Ping Lobanov, Andrei P. Loinard, Laurent Lonsdale, Colin Lu, Ru-Sen MacDonald, Nicholas R. Mao, Jirong Markoff, Sera Marrone, Daniel P. Marscher, Alan P. Marti-Vidal, Ivan Matsushita, Satoki Matthews, Lynn D. Medeiros, Lia Menten, Karl M. Mizuno, Yosuke Mizuno, Izumi Moran, James M. Moriyama, Kotaro Moscibrodzka, Monika Muller, Cornelia Nagai, Hiroshi Nagar, Neil M. Nakamura, Masanori Narayan, Ramesh Narayanan, Gopal Natarajan, Iniyan Neri, Roberto Ni, Chunchong Noutsos, Aristeidis Okino, Hiroki Olivares, Hector Oyama, Tomoaki Ozel, Feryal Palumbo, Daniel C. M. Patel, Nimesh Pen, Ue-Li Pesce, Dominic W. Pietu, Vincent Plambeck, Richard PopStefanija, Aleksandar Porth, Oliver Prather, Ben Preciado-Lopez, Jorge A. Psaltis, Dimitrios Pu, Hung-Yi Ramakrishnan, Venkatessh Rao, Ramprasad Rawlings, Mark G. Raymond, Alexander W. Rezzolla, Luciano Ripperda, Bart Roelofs, Freek Rogers, Alan Ros, Eduardo Rose, Mel Roshanineshat, Arash Rottmann, Helge Roy, Alan L. Ruszczyk, Chet Ryan, Benjamin R. Rygl, Kazi L. J. Sanchez, Salvador Sanchez-Arguelles, David Sasada, Mahito Savolainen, Tuomas Schloerb, F. Peter Schuster, Karl-Friedrich Shao, Lijing Shen, Zhiqiang Small, Des Sohn, Bong Won SooHoo, Jason Tazaki, Fumie Tiede, Paul Tilanus, Remo P. J. Titus, Michael Toma, Kenji Torne, Pablo Trent, Tyler Trippe, Sascha Tsuda, Shuichiro van Bemmel, Ilse van Langevelde, Huib Jan van Rossum, Daniel R. Wagner, Jan Wardle, John Weintroub, Jonathan Wex, Norbert Wharton, Robert Wielgus, Maciek Wong, George N. Wu, Qingwen Young, Andre Young, Ken Younsi, Ziri Yuan, Feng Yuan, Ye-Fei Zensus, J. Anton Zhao, Guangyao Zhao, Shan-Shan Zhu, Ziyan Anczarski, Jadyn Baganoff, Frederick K. Eckart, Andreas Farah, Joseph R. Haggard, Daryl Meyer-Zhao, Zheng Michalik, Daniel Nadolski, Andrew Neilsen, Joseph Nishioka, Hiroaki Nowak, Michael A. Pradel, Nicolas Primiani, Rurik A. Souccar, Kamal Vertatschitsch, Laura Yamaguchi, Paul Zhang, Shuo |
| Affiliation | Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA MIT, Haystack Observ, 99 Millstone Rd, Westford, MA 01886 USA Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan Harvard Univ, Black Hole Initiat, 20 Garden St, Cambridge, MA 02138 USA CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany Acad Sinica, Inst Astron & Astrophys, 11F Astron Math Bldg,AS NTU 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan Univ Valencia, Dept Astron & Astrofis, C Dr Moliner 50, E-46100 Valencia, Spain Univ Valencia, Observ Astron, C Catedrat Jose Beltran 2, E-46980 Valencia, Spain Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA Univ Arizona, Dept Astron, 933 N Cherry Ave, Tucson, AZ 85721 USA Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA East Asian Observ, 660 N Aohoku Pl, Hilo, HI 96720 USA Nederlandse Onderzoekschool Astron 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| Keywords | accretion, accretion disks black hole physics galaxies: individual (M87) galaxies: jets magnetohydrodynamics (MHD) techniques: high angular resolution |
| Issue Date | 2019 |
| Publisher | ASTROPHYSICAL JOURNAL LETTERS |
| Abstract | The Event Horizon Telescope (EHT) has mapped the central compact radio source of the elliptical galaxy M87 at 1.3 mm with unprecedented angular resolution. Here we consider the physical implications of the asymmetric ring seen in the 2017 EHT data. To this end, we construct a large library of models based on general relativistic magnetohydrodynamic (GRMHD) simulations and synthetic images produced by general relativistic ray tracing. We compare the observed visibilities with this library and confirm that the asymmetric ring is consistent with earlier predictions of strong gravitational lensing of synchrotron emission from a hot plasma orbiting near the black hole event horizon. The ring radius and ring asymmetry depend on black hole mass and spin, respectively, and both are therefore expected to be stable when observed in future EHT campaigns. Overall, the observed image is consistent with expectations for the shadow of a spinning Kerr black hole as predicted by general relativity. If the black hole spin and M87's large scale jet are aligned, then the black hole spin vector is pointed away from Earth. Models in our library of non-spinning black holes are inconsistent with the observations as they do not produce sufficiently powerful jets. At the same time, in those models that produce a sufficiently powerful jet, the latter is powered by extraction of black hole spin energy through mechanisms akin to the Blandford-Znajek process. We briefly consider alternatives to a black hole for the central compact object. Analysis of existing EHT polarization data and data taken simultaneously at other wavelengths will soon enable new tests of the GRMHD models, as will future EHT campaigns at 230 and 345 GHz. |
| URI | http://hdl.handle.net/20.500.11897/549149 |
| ISSN | 2041-8205 |
| DOI | 10.3847/2041-8213/ab0f43 |
| Indexed | SCI(E) EI |
| Appears in Collections: | 物理学院 科维理天文与天体物理研究所 |
