Relative Astrometry of Compact Flaring Structures in Sgr A* with Polarimetric VLBI
arXiv:1408.6241 · doi:10.1088/0004-637X/794/2/150
Abstract
We demonstrate that polarimetric interferometry can be used to extract precise spatial information about compact polarized flares of Sgr A*. We show that, for a faint dynamical component, a single interferometric baseline suffices to determine both its polarization and projected displacement from the quiescent intensity centroid. A second baseline enables two-dimensional reconstruction of the displacement, and additional baselines can self-calibrate using the flare, enhancing synthesis imaging of the quiescent emission. We apply this technique to simulated 1.3-mm wavelength observations of a "hot spot" embedded in a radiatively inefficient accretion disk around Sgr A*. Our results indicate that, even with current sensitivities, polarimetric interferometry with the Event Horizon Telescope can achieve ~5 microarcsecond relative astrometry of compact flaring structures near Sgr A* on timescales of minutes.
9 Pages, 4 Figures, accepted for publication in ApJ
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Cited by in corpus (6)
- The Event Horizon Telescope: exploring strong gravity and accretion physics
- Dynamical Imaging with Interferometry
- Demonstrating Photon Ring Existence with Single-Baseline Polarimetry
- Forward Ray Tracing and Hot Spots in Kerr Spacetime
- Probing the Spacetime Around Supermassive Black Holes with Ejected Plasma Blobs
- Investigating the Disk-Jet Structure in M87 through Flux Separation in the Linear and Circular Polarization Images