MOJAVE XXI. Decade-long linear polarization variability in AGN jets at parsec scales

Abstract

Using stacking of images obtained at different epochs, we studied the variability properties of linear polarization of active galactic nucleus (AGN) jets on parsec-scales. Our sample is drawn from the MOJAVE programme, and consists of 436 AGNs manifesting core-jet morphology and having at least five VLBA observing epochs at 15 GHz from January 1996 through August 2019, with some additional archival VLBA data reduced by us. We employed a stacking procedure and constructed maps of (i) standard deviation of fractional polarization and electric vector position angle (EVPA) over epochs as the measure of variability and (ii) median polarization degree to quantify typical values in time. The distributions of these values along and across the jet were analysed for the whole sample for the first time. We found that core EVPA variability is typically higher than that of the jet, presumably due to component blending and outflow bends in the core. The BL Lacertae object cores have lower EVPA variability, compared to that of quasars, possibly due to lower Faraday rotation measure, suggesting a stronger ordered magnetic field component. The EVPA becomes more stable down the jet. Most of the sources showing this trend have a time coverage of more than 12 years and at least 15 epochs. The possible cause could be the increase of stability in the magnetic field direction, reflecting an increase in the fraction of the magnetic field that is ordered. There are no significant optical-class-dependent or spectral-class-dependent relations in the EVPA variability properties in AGN jets.

15 pages, 11 figures, 5 tables; accepted by MNRAS; full electronic tables are available as ancillary files

References in corpus (15)

• MOJAVE: Monitoring of Jets in AGN with VLBA Experiments. V. Multi-epoch VLBA Images
• MOJAVE: XV. VLBA 15 GHz Total Intensity and Polarization Maps of 437 Parsec-Scale AGN Jets From 1996-2017
• MOJAVE. XVII. Jet Kinematics and Parent Population Properties of Relativistically Beamed Radio-Loud Blazars
• MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VIII. Faraday rotation in parsec-scale AGN jets
• The VLBA Imaging and Polarimetry Survey at 5 GHz
• MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. XI. Spectral distributions
• MOJAVE: XVIII. Kinematics and Inner Jet Evolution of Bright Radio-Loud Active Galaxies
• Three dimensional magnetic field structure of six parsec-scale active galactic nuclei jets
• Are Spine--Sheath Polarization Structures in the Jets of Active Galactic Nuclei Associated with Helical Magnetic Fields?
• Transverse Faraday-Rotation Gradients Across the Jets of 15 Active Galactic Nuclei
• MOJAVE. XX. Persistent Linear Polarization Structure in Parsec-scale AGN Jets
• Parsec Scale Faraday-Rotation Structure Across the Jets of 9 Active Galactic Nuclei
• An oversized magnetic sheath wrapping around the parsec-scale jet in 3C 273
• The University of Michigan Centimeter-Band All Stokes Blazar Monitoring Program: Single-Dish Polarimetry as a Probe of Parsec-Scale Magnetic Fields
• Polarization Observations of AGN Jets: Past and Future

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• Looking into the Jet Cone of the Neutrino-Associated Very High Energy Blazar PKS 1424+240
• Depolarization and Faraday effects in AGN Jets
• Kilogauss magnetic field and jet dynamics in the quasar NRAO 530
• Probing circular polarization and magnetic field structure in AGN
• Simulations of linear polarization of precessing AGN jets at parsec scales