• DOI:10.1051/0004-6361/202244493
• Corpus ID: 252408562

Orbital motion near Sagittarius A*

@article{Wielgus2022OrbitalMN,
  title={Orbital motion near Sagittarius A*},
  author={Maciek Wielgus and Monika A. Mościbrodzka and Jesse Vos and Zachary Gelles and Iv{\'a}n Mart{\'i}-Vidal and Joseph R. Farah and Nicola Marchili and Ciriaco Goddi and Hugo Messias},
  journal={Astronomy \& Astrophysics},
  year={2022}
}

• M. Wielgus, M. Mościbrodzka, +6 authors H. Messias
• Published 1 September 2022
• Physics
• Astronomy & Astrophysics

We report on the polarized light curves of the Galactic Center supermassive black hole Sagittarius A*, obtained at millimeter wavelength with the Atacama Large Millimeter/submillimeter Array (ALMA). The observations took place as a part of the Event Horizon Telescope campaign. We compare the observations taken during the low variability source state on 2017 Apr. 6 and 7 with those taken immediately after the X-ray flare on 2017 Apr. 11. For the latter case, we observe rotation of the electric vector position angle with a timescale of ∼70 min. We interpret this rotation as a signature of the equatorial clockwise orbital motion of a hot spot embedded in a magnetic field dominated by a dynamically important vertical component, observed at a low inclination ∼20°. The hot spot radiates strongly polarized synchrotron emission, briefly dominating the linear polarization measured by ALMA in the unresolved source. Our simple emission model captures the overall features of the polarized light curves remarkably well. Assuming a Keplerian orbit, we find the hot spot orbital radius to be ∼5 Schwarzschild radii. We observe hints of a positive black hole spin, that is, a prograde hot spot motion. Accounting for the rapidly varying rotation measure, we estimate the projected on-sky axis of the angular momentum of the hot spot to be ∼60° east of north, with a 180° ambiguity. These results suggest that the accretion structure in Sgr A* is a magnetically arrested disk rotating clockwise.