Monitoring the Morphology of M87* in 2009-2017 with the Event Horizon Telescope
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- Harvard U.; Harvard-Smithsonian Ctr. Astrophys.
- NRAO, Charlottesville; MIT, Haystack Observ.; Natl. Astron. Observ. of Japan; Harvard U.
- Arizona U., Astron. Dept. - Steward Observ.
- Colorado U.; JILA, Boulder
- MIT, Haystack Observ.
- Nijmegen U., IMAPP
- Bonn, Max Planck Inst., Radioastron.
- Shanghai, Astron. Observ.; Bonn, Max Planck Inst., Radioastron.
- Illinois U., Urbana; Los Alamos
- Inst. Astron. Astrophys., Hilo
- Perimeter Inst. Theor. Phys.; Waterloo U.
- Princeton U., PCTS; NASA, Marshall
- Amsterdam U., Astron. Inst.
- Illinois U., Urbana; Illinois U., Urbana, Astron. Dept.
- Waterloo U.
- Natl. Astron. Observ. of Japan; Sokendai, Tsukuba
- Mexico U.; UNAM, Morelia, CCM; UNAM, Inst. Astron.
- Amsterdam U., Astron. Inst.; U. Amsterdam, GRAPPA
- UC, Berkeley
- IAA, Granada
- Taiwan, Natl. Taiwan U.
- Valencia U., Astro. Astrophys.; Valencia U., IFIC; Bonn, Max Planck Inst., Radioastron.
- INFN, Trieste; SISSA, Trieste; Trieste U.
- East Asian Observ.
- Leiden Observ.
- Harvard U.; Harvard-Smithsonian Ctr. Astrophys.; Caltech
- IRAM, St. Martin d'Heres
- KASI, DaeJeon; KAIST, Taejon
- Chicago U., KICP; Chicago U., Astron. Astrophys. Ctr.; Chicago U.; Chicago U., EFI
- Cornell U., Radio. Space Res. Ctr.
- Shanghai, Astron. Observ.; Key Lab. Radio Astron., Nanjing
- Arizona U., Astron. Dept. - Steward Observ.; Harvard-Smithsonian Ctr. Astrophys.
- Onsala Space Observ.
- Naples U.; Frankfurt U.; INFN, Naples
- Pretoria U.; Rhodes U.
- LESIA, Meudon
- NRAO, Charlottesville
- Frankfurt U.
- Harvard U.
- Nijmegen U., IMAPP; Leiden Observ.
- Southern Denmark U., CP3-Origins; Perimeter Inst. Theor. Phys.
- INAOE, Puebla; Conacyt, Mexico
- Shanghai, Astron. Observ.
- Harvard-Smithsonian Ctr. Astrophys.
- Groningen, KVI
- Peking U.; Peking U., Beijing, KIAA
- INAOE, Puebla
- Fermilab
- Garching, Max Planck Inst., MPE
- Boston U.; St. Petersburg State U.
- Natl. Astron. Observ. of Japan
- JIVE, Dwingeloo
- Arizona U., Astron. Dept. - Steward Observ.; Caltech
- KASI, DaeJeon
- Natl. Astron. Observ. of Japan; Kogakuin U.
- Taiwan, Natl. Cheng Kung U.
- NRAO, Tucson
- Beijing, Inst. High Energy Phys.
- Nanjing U., Dept. Astron.; Nanjing U.
- Bologna Observ.
- Yunnan Observ.; CAMS-CAS, Beijing
- Bologna Observ.; Bonn, Max Planck Inst., Radioastron.
- Boston U.
- Valencia U., Astro. Astrophys.; Valencia U., IFIC
- Princeton, Inst. Advanced Study; Arizona U., Astron. Dept. - Steward Observ.
- Frankfurt U.; Shanghai Jiao Tong U.
- MIT, Haystack Observ.; Natl. Astron. Observ. of Japan
- Bonn, Max Planck Inst., Radioastron.; Nijmegen U., IMAPP
- Amsterdam U., Astron. Inst.; Nijmegen U., IMAPP
- Concepcion U.
- Massachusetts U., Amherst
- Rhodes U.
- Natl. Astron. Observ. of Japan; Tokyo U.
- Perimeter Inst. Theor. Phys.; Canadian Inst. Theor. Astrophys.; U. Toronto, Dunlap Inst. Astron. Astrophys.; Canadian Inst. Advanced Res.
- Amsterdam U., Astron. Inst.; Frankfurt U.
- Illinois U., Urbana
- Perimeter Inst. Theor. Phys.
- Perimeter Inst. Theor. Phys.; Taiwan, Natl. Normal U.; Taiwan, Natl. Taiwan U.
- Frankfurt U.; Trinity Coll., Dublin
- Princeton U., Astrophys. Sci. Dept.; Flatiron Inst., New York
- Los Alamos
- IRAM, Granada
- Natl. Astron. Observ. of Japan; Hiroshima U., HASC
- Aalto U.; Bonn, Max Planck Inst., Radioastron.
- Bonn, Max Planck Inst., Radioastron.; Peking U., Beijing, KIAA
- KASI, DaeJeon; KAIST, Taejon; Yonsei U.
- Nijmegen U., IMAPP; Leiden Observ.; NWO, The Hague; Nikhef, Amsterdam; Arizona U., Astron. Dept. - Steward Observ.
- Tohoku U., IIAIR; Tohoku U., Astron. Inst.
- Bonn, Max Planck Inst., Radioastron.; IRAM, Granada
- Seoul Natl. U., Dept. Phys. Astron.
- JIVE, Dwingeloo; Leiden Observ.
- Brandeis U.
- Central Lancashire U.
- Hua-Zhong U. Sci. Tech.
- Mullard Space Sci. Lab.; Frankfurt U.
- Shanghai, Astron. Observ.; Beijing, GUCAS
- Hefei, CUST
- Nijmegen U., IMAPP; Nanjing U., Dept. Astron.
The Event Horizon Telescope (EHT) has recently delivered the first resolved images of M87*, the supermassive black hole in the center of the M87 galaxy. These images were produced using 230 GHz observations performed in 2017 April. Additional observations are required to investigate the persistence of the primary image feature—a ring with azimuthal brightness asymmetry—and to quantify the image variability on event horizon scales. To address this need, we analyze M87* data collected with prototype EHT arrays in 2009, 2011, 2012, and 2013. While these observations do not contain enough information to produce images, they are sufficient to constrain simple geometric models. We develop a modeling approach based on the framework utilized for the 2017 EHT data analysis and validate our procedures using synthetic data. Applying the same approach to the observational data sets, we find the M87* morphology in 2009–2017 to be consistent with a persistent asymmetric ring of ∼40 μas diameter. The position angle of the peak intensity varies in time. In particular, we find a significant difference between the position angle measured in 2013 and 2017. These variations are in broad agreement with predictions of a subset of general relativistic magnetohydrodynamic simulations. We show that quantifying the variability across multiple observational epochs has the potential to constrain the physical properties of the source, such as the accretion state or the black hole spin.
- Research Organization:
- UC, Berkeley; Peking U.; MIT, Haystack Observ.; Natl. Astron. Observ. of Japan; SISSA, Trieste; Illinois U., Urbana; IRAM, St. Martin d'Heres; Shanghai, Astron. Observ.; Princeton U., Astrophys. Sci. Dept.; Brandeis U.; Boston U.; Taiwan, Natl. Cheng Kung U.; Flatiron Inst., New York; Nanjing U.; Nijmegen U., IMAPP; Valencia U., IFIC; Trinity Coll., Dublin; Groningen, KVI; Waterloo U.; Taiwan, Natl. Normal U.; INFN, Trieste; Onsala Space Observ.; IRAM, Granada; Beijing, Inst. High Energy Phys.; Peking U., Beijing, KIAA; East Asian Observ.; Mexico U.; Taiwan, Natl. Taiwan U.; Chicago U., Astron. Astrophys. Ctr.; Tokyo U.; Cornell U., Radio. Space Res. Ctr.; NWO, The Hague; Beijing, GUCAS; Yonsei U.; Pretoria U.; Naples U.; LESIA, Meudon; Bologna Observ.; Valencia U., Astro. Astrophys.; CAMS-CAS, Beijing; Chicago U., KICP; Inst. Astron. Astrophys., Hilo; Concepcion U.; Yunnan Observ.; Chicago U.; NRAO, Charlottesville; NRAO, Tucson; U. Toronto, Dunlap Inst. Astron. Astrophys.; INAOE, Puebla; Sokendai, Tsukuba; Leiden Observ.; INFN, Naples; Trieste U.; JILA, Boulder; Harvard U.; Hefei, CUST; KAIST, Taejon; JIVE, Dwingeloo; Arizona U., Astron. Dept. - Steward Observ.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); St. Petersburg State U.; KASI, DaeJeon; Southern Denmark U., CP3-Origins; Perimeter Inst. Theor. Phys.; Garching, Max Planck Inst., MPE; Kogakuin U.; Conacyt, Mexico; Seoul Natl. U., Dept. Phys. Astron.; Massachusetts U., Amherst; Chicago U., EFI; Frankfurt U.; Central Lancashire U.; Key Lab. Radio Astron., Nanjing; Canadian Inst. Theor. Astrophys.; Rhodes U.; Caltech; NASA, Marshall; Shanghai Jiao Tong U.; Mullard Space Sci. Lab.; Bonn, Max Planck Inst., Radioastron.; Hua-Zhong U. Sci. Tech.; IAA, Granada; Harvard-Smithsonian Ctr. Astrophys.; Hiroshima U., HASC; Princeton U., PCTS; Amsterdam U., Astron. Inst.; Nikhef, Amsterdam; U. Amsterdam, GRAPPA; UNAM, Inst. Astron.; Tohoku U., Astron. Inst.; Princeton, Inst. Advanced Study; Colorado U.; UNAM, Morelia, CCM; Illinois U., Urbana, Astron. Dept.; Canadian Inst. Advanced Res.; Aalto U.; Nanjing U., Dept. Astron.; Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Tohoku U., IIAIR
- Sponsoring Organization:
- US Department of Energy
- Grant/Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1674987
- Alternate ID(s):
- OSTI ID: 2426556
OSTI ID: 23031328
- Report Number(s):
- FERMILAB-PUB-20-534-V; oai:inspirehep.net:1818905; arXiv:2009.11842
- Journal Information:
- Astrophys.J., Journal Name: Astrophys.J. Journal Issue: 1 Vol. 901
- Country of Publication:
- United States
- Language:
- English
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