Are Spine--Sheath Polarization Structures in the Jets of Active Galactic Nuclei Associated with Helical Magnetic Fields?
Denise C. Gabuzda, Andrea Reichstein, Eamonn L. O'Neill

TL;DR
This study investigates whether spine--sheath polarization structures in AGN jets are linked to helical magnetic fields by analyzing polarization and Faraday rotation gradients across multiple frequencies.
Contribution
It provides observational evidence supporting the association between spine--sheath polarization structures and helical magnetic fields in AGN jets, including detection of transverse Faraday rotation gradients and their reversals.
Findings
Detection of monotonic transverse Faraday rotation gradients in 8 AGNs.
Reversals of RM gradient directions suggest nested helical magnetic fields.
Results support the presence of helical magnetic fields in AGN jets.
Abstract
One possible origin for polarization structures across jets of Active Galactic Nuclei (AGNs) with a central "spine" of orthogonal magnetic field and a "sheath" of longitudinal magnetic field along one or both edges of the jet is the presence of a helical jet magnetic field. Simultaneous Very Long Baseline Array (VLBA) polarization observations of AGN displaying partial or full spine--sheath polarization structures were obtained at 4.6, 5.0, 7.9, 8.9, 12.9 and 15.4 GHz, in order to search for additional evidence for helical jet magnetic fields, such as transverse Faraday rotation gradients (due to the systematic change in the line-of-sight magnetic-field component across the jet). Results for eight sources displaying monotonic transverse Faraday rotation gradients with significances are presented here. Reversals in the directions of the transverse RM gradients with…
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