Horizon-scale variability of M87* from 2017–2021 EHT observations
Kazunori Akiyama;Ezequiel Albentosa-Ru??z;Antxon Alberdi;Walter Alef;Juan Carlos Algaba;Richard Anantua;Keiichi Asada;Rebecca Azulay;Uwe Bach;Anne-Kathrin Baczko;David Ball;Mislav Balokovi??;Bidisha Bandyopadhyay;John Barrett;Michi Baub??ck;Bradford A. Benson;Dan Bintley;Lindy Blackburn;Raymond Blundell;Katherine L. Bouman;Geoffrey C. Bower;Michael Bremer;Roger Brissenden;Silke Britzen;Avery E. Broderick;Dominique Broguiere;Thomas Bronzwaer;Sandra Bustamante;Douglas F. Carlos;John E. Carlstrom;Andrew Chael;Chi-kwan Chan;Dominic O. Chang;Erandi Chavez;Koushik Chatterjee;Shami Chatterjee;Ming-Tang Chen;Yongjun Chen;Xiaopeng Cheng;Paul Chichura;Ilje Cho;Pierre Christian;Nicholas S. Conroy;John E. Conway;Thomas M. Crawford;Geoffrey B. Crew;Alejandro Cruz-Osorio;Yuzhu Cui;Brandon Curd;Rohan Dahale;Jordy Davelaar;Mariafelicia De Laurentis;Roger Deane;Gregory Desvignes;Jason Dexter;Vedant Dhruv;Indu K. Dihingia;Sheperd S. Doeleman;Sergio A. Dzib;Ralph P. Eatough;Razieh Emami;Heino Falcke;Joseph Farah;Vincent L. Fish;Edward Fomalont;H. Alyson Ford;Marianna Foschi;Raquel Fraga-Encinas;William T. Freeman;Per Friberg;Christian M. Fromm;Antonio Fuentes;Peter Galison;Charles F. Gammie;Roberto Garc??a;Olivier Gentaz;Boris Georgiev;Ciriaco Goddi;Roman Gold;Arturo I. G??mez-Ruiz;Jos?? L. G??mez;Minfeng Gu;Mark Gurwell;Kazuhiro Hada;Daryl Haggard;Ronald Hesper;Dirk Heumann;Luis C. Ho;Paul Ho;Dan Hoak;Mareki Honma;Chih-Wei L. Huang;Lei Huang;David H. Hughes;Shiro Ikeda;C. M. Violette Impellizzeri;Makoto Inoue;Sara Issaoun;David J. James;Buell T. Jannuzi;Michael Janssen;Britton Jeter;Wu Jiang;Alejandra Jim??nez-Rosales;Michael D. Johnson;Svetlana Jorstad;Adam C. Jones;Abhishek V. Joshi;Taehyun Jung;Ramesh Karuppusamy;Tomohisa Kawashima;Garrett K. Keating;Mark Kettenis;Dong-Jin Kim;Jae-Young Kim;Jongsoo Kim;Junhan Kim;Motoki Kino;Jun Yi Koay;Prashant Kocherlakota;Yutaro Kofuji;Patrick M. Koch;Shoko Koyama;Carsten Kramer;Joana A. Kramer;Michael Kramer;Thomas P. Krichbaum;Cheng-Yu Kuo;Noemi La Bella;Deokhyeong Lee;Sang-Sung Lee;Aviad Levis;Zhiyuan Li;Rocco Lico;Greg Lindahl;Michael Lindqvist;Mikhail Lisakov;Jun Liu;Kuo Liu;Elisabetta Liuzzo;Wen-Ping Lo;Andrei P. Lobanov;Laurent Loinard;Colin J. Lonsdale;Amy E. Lowitz;Ru-Sen Lu;Nicholas R. MacDonald;Jirong Mao;Nicola Marchili;Sera Markoff;Daniel P. Marrone;Alan P. Marscher;Iv??n Mart??-Vidal;Satoki Matsushita;Lynn D. Matthews;Lia Medeiros;Karl M. Menten;Izumi Mizuno;Yosuke Mizuno;Joshua Montgomery;James M. Moran;Kotaro Moriyama;Monika Moscibrodzka;Wanga Mulaudzi;Cornelia M??ller;Hendrik M??ller;Alejandro Mus;Gibwa Musoke;Ioannis Myserlis;Hiroshi Nagai;Neil M. Nagar;Dhanya G. Nair;Masanori Nakamura;Gopal Narayanan;Iniyan Natarajan;Antonios Nathanail;Santiago Navarro Fuentes;Joey Neilsen;Chunchong Ni;Michael A. Nowak;Junghwan Oh;Hiroki Okino;H??ctor Ra??l Olivares S??nchez;Tomoaki Oyama;Feryal ??zel;Daniel C. M. Palumbo;Georgios Filippos Paraschos;Jongho Park;Harriet Parsons;Nimesh Patel;Ue-Li Pen;Dominic W. Pesce;Vincent Pi??tu;Alexander Plavin;Aleksandar PopStefanija;Oliver Porth;Ben Prather;Giacomo Principe;Dimitrios Psaltis;Hung-Yi Pu;Alexandra Rahlin;Venkatessh Ramakrishnan;Ramprasad Rao;Mark G. Rawlings;Luciano Rezzolla;Angelo Ricarte;Luca Ricci;Bart Ripperda;Jan R??der;Freek Roelofs;Cristina Romero-Ca??izales;Eduardo Ros;Arash Roshanineshat;Helge Rottmann;Alan L. Roy;Ignacio Ruiz;Chet Ruszczyk;Kazi L. J. Rygl;Le??n D. S. Salas;Salvador S??nchez;David S??nchez-Arg??elles;Miguel S??nchez-Portal;Mahito Sasada;Kaushik Satapathy;Saurabh;Tuomas Savolainen;F. Peter Schloerb;Jonathan Schonfeld;Karl-Friedrich Schuster;Lijing Shao;Zhiqiang Shen;Sasikumar Silpa;Des Small;Randall Smith;Bong Won Sohn;Jason SooHoo;Kamal Souccar;Joshua S. Stanway;He Sun;Fumie Tazaki;Alexandra J. Tetarenko;Paul Tiede;Remo P. J. Tilanus;Michael Titus;Kenji Toma;Pablo Torne;Teresa Toscano;Efthalia Traianou;Tyler Trent;Sascha Trippe;Matthew Turk;Ilse van Bemmel;Huib Jan van Langevelde;Daniel R. van Rossum;Sebastiano D. von Fellenberg;Jesse Vos;Jan Wagner;Derek Ward-Thompson;John Wardle;Jasmin E. Washington;Jonathan Weintroub;Andrew T. West;Robert Wharton;Maciek Wielgus;Kaj Wiik;Gunther Witzel;Michael F. Wondrak;George N. Wong;Jompoj Wongphexhauxsorn;Qingwen Wu;Nitika Yadlapalli;Paul Yamaguchi;Aristomenis Yfantis;Doosoo Yoon;Andr?? Young;Ziri Younsi;Wei Yu;Feng Yuan;Ye-Fei Yuan;Ai-Ling Zeng;J. Anton Zensus;Shuo Zhang;Guang-Yao Zhao;Shan-Shan Zhao;Ryan Berthold;Shu-Hao Chang;Ryan Chilson;Chih-Chiang Han;David M. Gale;Gertie Geertsema;Jos?? Luis Hern??ndez-Rebollar;Yau-De Huang;Ryan P. Keenan;Derek Kubo;Kuan-Yu Liu;Pierre L. Martin-Cocher;Daniel Michalik;Alfredo Monta??a;Andrew Nadolski;Peter Oshiro;Philippe A. Raffin;Iv??n Rodr??guez-Montoya;Ta-Shun Wei;Matthew R. Young
2025-01-01
Abstract
We report three epochs of polarized images of M87* at 230 GHz using data from the Event Horizon Telescope (EHT) taken in 2017, 2018, and 2021. The baseline coverage of the 2021 observations is significantly improved through the addition of two new EHT stations: the 12 m Kitt Peak Telescope and the Northern Extended Millimetre Array (NOEMA). All observations result in images dominated by a bright, asymmetric ring with a persistent diameter of 43.9 ± 0.6 µas, consistent with expectations for lensed synchrotron emission encircling the apparent shadow of a supermassive black hole. We find that the total intensity and linear polarization of M87* vary significantly across the three epochs. Specifically, the azimuthal brightness distribution of the total intensity images varies from year to year, as expected for a stochastic accretion flow. However, despite a gamma-ray flare erupting in M87 quasi-contemporaneously to the 2018 observations, the 2018 and 2021 images look remarkably similar. The resolved linear polarization fractions in 2018 and 2021 peak at ∼5%, compared to ∼15% in 2017. The spiral polarization pattern on the ring also varies from year to year, including a change in the electric vector position angle helicity in 2021 that could reflect changes in the magnetized accretion flow or an external Faraday screen. The improved 2021 coverage also provides the first EHT constraints on jet emission outside the ring, on scales of .1 mas. Overall, these observations provide strong proof of the reliability of the EHT images and probe the dynamic properties of the horizon-scale accretion flow surrounding M87*.