High-Sensitivity AGN Polarimetry at Sub-Millimeter Wavelengths
The innermost regions of radio loud Active Galactic Nuclei (AGN) jets are heavily affected by synchrotron self-absorption, due to the strong magnetic fields and high particle densities in these extreme zones. The only way to overcome this absorption is to observe at sub-millimeter wavelengths, altho...
Main Authors: | Ivan Martí-Vidal, Sébastien Muller |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2017-10-01
|
Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/5/4/65 |
Similar Items
-
Linear Polarization Properties of Parsec-Scale AGN Jets
by: Alexander B. Pushkarev, et al.
Published: (2017-12-01) -
Evidence for Toroidal B-Field Components in AGN Jets on Kiloparsec Scales
by: Sebastian Knuettel, et al.
Published: (2017-10-01) -
The Origin and Structure of the Magnetic Fields and Currents of AGN Jets
by: Denise Gabuzda
Published: (2017-02-01) -
Determining the Jet Poloidal B Field and Black-Hole Rotation Directions in AGNs
by: Denise Gabuzda
Published: (2018-01-01) -
Evidence for Helical Magnetic Fields Associated with AGN Jets and the Action of a Cosmic Battery
by: Denise Gabuzda
Published: (2018-12-01)