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....
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-07-01
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Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/9/3/51 |