High-Frequency Polarization Variability from Active Galactic Nuclei

The linear polarization of non-thermal emission encodes information about the structure of the magnetic fields, either from the region where the emission is produced (i.e., the intrinsic polarization angle) and/or from the screens of magnetized plasma that may be located on its way towards Earth (i....

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Bibliographic Details
Main Authors: Iván Martí-Vidal, Ciriaco Goddi
Format: Article
Language:English
Published: MDPI AG 2021-07-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/9/3/51