Supermassive Black Hole Spin Constraints from Polarimetry in an Equatorial Disk Model

The Event Horizon Telescope has released polarized images of the supermassive black holes Messier 87* (M87*) and Sagittarius A* accretion disks. As more images are produced, our understanding of the average polarized emission from near the event horizon improves. In this Letter, we use a semianalyti...

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Bibliographic Details
Main Author: Daniel C. M. Palumbo
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/ad9bb4
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