The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A*
The ring-like images of the two supermassive black holes captured by the Event Horizon Telescope (EHT) provide powerful probes of the physics of accretion flows at horizon scales. Specifically, the brightness asymmetry in the images carries information about the angular velocity profile of the inner...
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IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
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| Online Access: | https://doi.org/10.3847/1538-4357/ad9689 |
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| author | J. Cole Faggert Feryal Özel Dimitrios Psaltis |
| author_facet | J. Cole Faggert Feryal Özel Dimitrios Psaltis |
| author_sort | J. Cole Faggert |
| collection | DOAJ |
| description | The ring-like images of the two supermassive black holes captured by the Event Horizon Telescope (EHT) provide powerful probes of the physics of accretion flows at horizon scales. Specifically, the brightness asymmetry in the images carries information about the angular velocity profile of the inner accretion flow and the inclination of the observer, owing to the Doppler boosts photons experience at their site of emission. In this paper, we develop a method for quantifying the brightness asymmetry of black hole images in the Fourier domain, which can be measured directly from interferometric data. We apply this method to current EHT data and find that the image of Sagittarius A* (Sgr A*) has an unusually low degree of asymmetry that is even lower than that inferred for M87. We then use a covariant semianalytic model to obtain constraints on the inclinations and velocity profiles of the inner accretion flow for Sgr A*. We find that the lack of significant brightness asymmetry forces the observer inclination to uncomfortably small values (6°–10 ^∘ ), if the plasma velocity follows Keplerian profiles. Alternatively, larger inclination angles can be accommodated if the plasma velocities are significantly sub-Keplerian and the black hole is not spinning rapidly. |
| format | Article |
| id | doaj-art-94caa0868fdc4a698a2f791bdee8bc2a |
| institution | DOAJ |
| issn | 1538-4357 |
| language | English |
| publishDate | 2025-01-01 |
| publisher | IOP Publishing |
| record_format | Article |
| series | The Astrophysical Journal |
| spelling | doaj-art-94caa0868fdc4a698a2f791bdee8bc2a2025-08-20T02:57:48ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01981220910.3847/1538-4357/ad9689The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A*J. Cole Faggert0https://orcid.org/0000-0003-4440-8924Feryal Özel1https://orcid.org/0000-0003-4413-1523Dimitrios Psaltis2https://orcid.org/0000-0003-1035-3240School of Physics, Georgia Institute of Technology , 837 State St. NW, Atlanta, GA 30332, USASchool of Physics, Georgia Institute of Technology , 837 State St. NW, Atlanta, GA 30332, USASchool of Physics, Georgia Institute of Technology , 837 State St. NW, Atlanta, GA 30332, USAThe ring-like images of the two supermassive black holes captured by the Event Horizon Telescope (EHT) provide powerful probes of the physics of accretion flows at horizon scales. Specifically, the brightness asymmetry in the images carries information about the angular velocity profile of the inner accretion flow and the inclination of the observer, owing to the Doppler boosts photons experience at their site of emission. In this paper, we develop a method for quantifying the brightness asymmetry of black hole images in the Fourier domain, which can be measured directly from interferometric data. We apply this method to current EHT data and find that the image of Sagittarius A* (Sgr A*) has an unusually low degree of asymmetry that is even lower than that inferred for M87. We then use a covariant semianalytic model to obtain constraints on the inclinations and velocity profiles of the inner accretion flow for Sgr A*. We find that the lack of significant brightness asymmetry forces the observer inclination to uncomfortably small values (6°–10 ^∘ ), if the plasma velocity follows Keplerian profiles. Alternatively, larger inclination angles can be accommodated if the plasma velocities are significantly sub-Keplerian and the black hole is not spinning rapidly.https://doi.org/10.3847/1538-4357/ad9689Supermassive black holesAccretionPlasma astrophysics |
| spellingShingle | J. Cole Faggert Feryal Özel Dimitrios Psaltis The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A* The Astrophysical Journal Supermassive black holes Accretion Plasma astrophysics |
| title | The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A* |
| title_full | The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A* |
| title_fullStr | The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A* |
| title_full_unstemmed | The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A* |
| title_short | The Unexpected Lack of Asymmetry in the Horizon-scale Image of Sagittarius A* |
| title_sort | unexpected lack of asymmetry in the horizon scale image of sagittarius a |
| topic | Supermassive black holes Accretion Plasma astrophysics |
| url | https://doi.org/10.3847/1538-4357/ad9689 |
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