Measuring the Direction and Angular Velocity of a Black Hole Accretion Disk via Lagged Interferometric Covariance
arXiv:1505.07870 · doi:10.1088/0004-637X/813/2/132
Abstract
We show that interferometry can be applied to study irregular, rapidly rotating structures, as are expected in the turbulent accretion flow near a black hole. Specifically, we analyze the lagged covariance between interferometric baselines of similar lengths but slightly different orientations. For a flow viewed close to face-on, we demonstrate that the peak in the lagged covariance indicates the direction and angular velocity of the emission pattern from the flow. Even for moderately inclined flows, the covariance robustly estimates the flow direction, although the estimated angular velocity can be significantly biased. Importantly, measuring the direction of the flow as clockwise or counterclockwise on the sky breaks a degeneracy in accretion disk inclinations when analyzing time-averaged images alone. We explore the potential efficacy of our technique using three-dimensional, general relativistic magnetohydrodynamic (GRMHD) simulations, and we highlight several baseline pairs for the Event Horizon Telescope (EHT) that are well-suited to this application. These results indicate that the EHT may be capable of estimating the direction and angular velocity of the emitting material near Sagittarius A*, and they suggest that a rotating flow may even be utilized to improve imaging capabilities.
8 Pages, 4 Figures, accepted for publication in ApJ
References in corpus (14)
- Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre
- Jet Launching Structure Resolved Near the Supermassive Black Hole in M87
- An Unambiguous Detection of Faraday Rotation in Sagittarius A*
- RadioAstron -- a Telescope with a Size of 300 000 km: Main Parameters and First Observational Results
- The Submillimeter Bump in Sgr A* from Relativistic MHD Simulations
- Simulating the Emission and Outflows from Accretion Disks
- Radio and Millimeter Monitoring of Sgr A*: Spectrum, Variability, and Constraints on the G2 Encounter
- Imaging the Supermassive Black Hole Shadow and Jet Base of M87 with the Event Horizon Telescope
- The Galactic Center cloud G2 and its gas streamer
- Imaging an Event Horizon: Mitigation of Scattering Toward Sagittarius A*
- Event-Horizon-Telescope Evidence for Alignment of the Black Hole in the Center of the Milky Way with the Inner Stellar Disk
- The Intrinsic Two-Dimensional Size of Sagittarius A*
- Discovery of Substructure in the Scatter-Broadened Image of Sgr A*
- Relative Astrometry of Compact Flaring Structures in Sgr A* with Polarimetric VLBI
Cited by in corpus (6)
- Sgr A* and General Relativity
- Modeling Seven Years of Event Horizon Telescope Observations with Radiatively Inefficient Accretion Flow Models
- Testing the No-Hair Theorem with Observations of Black Holes in the Electromagnetic Spectrum
- Probing the magnetic field structure in Sgr A* on Black Hole Horizon Scales with Polarized Radiative Transfer Simulations
- Dynamical Imaging with Interferometry
- Quantifying Intrinsic Variability of Sagittarius A* using Closure Phase Measurements of the Event Horizon Telescope