First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
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- Colorado U.
- Bonn, Max Planck Inst., Radioastron.; IRAM, St. Martin d'Heres
- Bonn, Max Planck Inst., Radioastron.; NAOC, Beijing
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We present the first Event Horizon Telescope (EHT) observations of Sagittarius A* (Sgr A*), the Galactic center source associated with a supermassive black hole. These observations were conducted in 2017 using a global interferometric array of eight telescopes operating at a wavelength of λ = 1.3 mm. The EHT data resolve a compact emission region with intrahour variability. A variety of imaging and modeling analyses all support an image that is dominated by a bright, thick ring with a diameter of 51.8 ± 2.3 μas (68% credible interval). The ring has modest azimuthal brightness asymmetry and a comparatively dim interior. Using a large suite of numerical simulations, we demonstrate that the EHT images of Sgr A* are consistent with the expected appearance of a Kerr black hole with mass ∼4 × 10$$^{6}$$ M $$_{⊙}$$, which is inferred to exist at this location based on previous infrared observations of individual stellar orbits, as well as maser proper-motion studies. Our model comparisons disfavor scenarios where the black hole is viewed at high inclination (i > 50°), as well as nonspinning black holes and those with retrograde accretion disks. Our results provide direct evidence for the presence of a supermassive black hole at the center of the Milky Way, and for the first time we connect the predictions from dynamical measurements of stellar orbits on scales of 10$$^{3}$$–10$$^{5}$$ gravitational radii to event-horizon-scale images and variability. Furthermore, a comparison with the EHT results for the supermassive black hole M87* shows consistency with the predictions of general relativity spanning over three orders of magnitude in central mass.
- Research Organization:
- ASTRON, Dwingeloo; Aalto U.; Academia Sinica, Taiwan; Americas U., Puebla; Arizona U.; Arizona U., Astron. Dept. - Steward Observ.; Athens U.; Baltimore, Space Telescope Sci.; Bard Coll.; Beijing, GUCAS; Bologna Observ.; Bologna, Ist. Radioastronomia; Bonn U.; Bonn, Max Planck Inst., Radioastron.; Boston U.; Brandeis U.; CCA, New York; Cagliari Observ.; Cagliari U.; Caltech; Canadian Inst. Advanced Res.; Canadian Inst. Theor. Astrophys.; Central Lancashire U.; Chalmers U. Tech.; Chicago U.; Chicago U., Astron. Astrophys. Ctr.; Chicago U., EFI; Chicago U., KICP; Chile U., Catolica; Colorado U.; Columbia U., Astron. Astrophys.; Conacyt, Mexico; Concepcion U.; Cornell U., Radio. Space Res. Ctr.; Drexel U.; ESTEC, Noordwijk; European Southern Obs., Chile; European Southern Observ.; Fairfield U.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Frankfurt U.; Frankfurt U., FIAS; Gemini Observ., Hilo; Google Inc.; Granada U., Theor. Phys. Astrophys.; Groningen U.; Hachinohe Inst. Tech.; Harvard U.; Harvard U. (main); Harvard U., Phys. Dept.; Harvard-Smithsonian Ctr. Astrophys.; Hawaii U.; Hefei, CUST; Hiroshima U.; Hong Kong, Chinese U.; Hua-Zhong U. Sci. Tech.; INAOE, Puebla; INFN, Naples; IRAM, Granada; IRAM, St. Martin d'Heres; Illinois U., Urbana; Illinois U., Urbana, Astron. Dept.; Jodrell Bank; KAIST, Taejon; KASI, DaeJeon; Kapteyn Astron. Inst., Groningen; Kogakuin U.; Kyungpook Natl. U.; LESIA, Meudon; Las Cumbres Observ.; Leiden Observ.; MIT; Malaya U.; Massachusetts U., Amherst; McGill U.; Mullard Space Sci. Lab.; NAOC, Beijing; NASA, Ames; NRAO, Charlottesville; NRAO, Socorro; NWO, The Hague; Nanjing U. Sci. Tech.; Nanjing U., Dept. Astron.; Naples U.; Natl. Astron. Observ. of Japan; Naval Research Lab, Wash., D.C.; Netherlands Meteorological Inst.; New Mexico U.; Niigata U.; Nijmegen U., IMAPP; Osaka Prefecture U.; Peking U.; Peking U., Beijing, KIAA; Perimeter Inst. Theor. Phys.; Pretoria U.; Princeton U.; Princeton U., Astrophys. Sci. Dept.; Princeton U., PCTS; Princeton, Inst. Advanced Study; Rhodes U.; Santa Barbara, KITP; Sejong U.; Seoul Natl. U.; Shanghai Jiaotong U.; Shanghai, Astron. Observ.; South African Astron. Observ.; Southern Denmark U., CP3-Origins; Subaru Telescope; Taiwan, Natl. Cheng Kung U.; Taiwan, Natl. Chiao Tung U.; Taiwan, Natl. Normal U.; Taiwan, Natl. Taiwan U.; Texas Tech. U., Lubbock; Texas U., San Antonio; Tokyo Inst. Tech.; Tokyo U.; Tokyo U., ICRR; Tokyo U., IPMU; Tokyo, Grad. U. Adv. Stud.; Tokyo, Inst. Statistical Math.; Toronto U., Astron. Dept.; Trinity Coll., Dublin; Tsung-Dao Lee Inst., Shanghai; Tuorla Observ.; Turku U.; U. Amsterdam, GRAPPA; U. Michigan, Dept. Astron.; U. Witwatersrand, Johannesburg, Sch. Phys.; UC, Berkeley; UC, Santa Barbara; UNAM, Inst. Astron.; UNAM, Morelia, Inst. Radioastron. Astrophys.; University Coll., Cork; Unlisted, US, MA; Valencia U., Astro. Astrophys.; Valencia U., IFIC; Vermont U.; Villanova U.; Washington U., St. Louis; Waterloo U.; Waterloo U., IQC; Western Ontario U.; Wurzburg U.; Yale Ctr. Astron. Astrophys.; Yonsei U.; Yunnan Observ.
- Sponsoring Organization:
- US Department of Energy
- Grant/Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1868453
- Report Number(s):
- FERMILAB-PUB-22-415-PPD; oai:inspirehep.net:2080889; arXiv:2311.08680
- Journal Information:
- Astrophys.J.Lett., Journal Name: Astrophys.J.Lett. Journal Issue: 2 Vol. 930
- Country of Publication:
- United States
- Language:
- English
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