Radiative Transfer Modeling of Radio-Band Linear Polarization Observations as a Probe of the Physical Conditions in the Jets of γ-Ray Flaring Blazars
Author:
Funder
National Science Foundation
NASA
Publisher
MDPI AG
Subject
Astronomy and Astrophysics
Link
http://www.mdpi.com/2075-4434/4/4/35/pdf
Reference20 articles.
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3. THE THIRD CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THEFERMILARGE AREA TELESCOPE
4. OBLIQUE SHOCKS AS THE ORIGIN OF RADIO TO GAMMA-RAY VARIABILITY IN ACTIVE GALACTIC NUCLEI
5. CONSTRAINING THE PHYSICAL CONDITIONS IN THE JETS OF γ-RAY FLARING BLAZARS USING CENTIMETER-BAND POLARIMETRY AND RADIATIVE TRANSFER SIMULATIONS. II. EXPLORING PARAMETER SPACE AND IMPLICATIONS
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1. Diagnosing Magnetic Field Geometry in Blazar Jets Using Multi-Frequency, Centimeter-Band Polarimetry and Radiative Transfer Modeling;Galaxies;2020-03-10
2. MOJAVE XVI: Multiepoch Linear Polarization Properties of Parsec-scale AGN Jet Cores;The Astrophysical Journal;2018-08-02
3. The University of Michigan Centimeter-Band All Stokes Blazar Monitoring Program: Single-Dish Polarimetry as a Probe of Parsec-Scale Magnetic Fields;Galaxies;2017-11-13
4. Observational View of Magnetic Fields in Active Galactic Nuclei Jets;Proceedings of the International Astronomical Union;2016-09
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