Parsec-scale Investigation of the Magnetic Field Structure of Several AGN Jets
Shane P. O'Sullivan, Denise C. Gabuzda

TL;DR
This study uses multi-frequency VLBA polarization observations to analyze the magnetic field structures of several AGN jets, revealing evidence of helical magnetic fields and variations in magnetic field orientation close to the central engine.
Contribution
It provides the first detailed multi-frequency polarization analysis of AGN jets, detecting transverse RM gradients and magnetic field changes indicative of helical magnetic structures.
Findings
Detection of transverse RM gradient in 0954+658 indicating a helical magnetic field.
Observation of RM sign changes in the core region across frequencies.
Magnetic field orientation is either parallel or perpendicular to the jet after Faraday correction.
Abstract
Multi-frequency (4.6, 5, 5.5, 8, 8.8, 13, 15, 22 & 43 GHz) polarization observations of 6 "blazars" were obtained on the American Very Long Baseline Array (VLBA) over a 24-hr period on 2 July 2006. Observing at several frequencies, separated by short and long intervals, enabled reliable determination of the distribution of Faraday Rotation on a range of scales. In all cases the magnitude of the RM increases in the higher frequency observations, implying that the electron density and/or magnetic field strength is increasing as we get closer to the central engine. After correcting for Faraday rotation, the polarization orientation in the jet is either parallel or perpendicular to the jet direction. A transverse Rotation Measure (RM) gradient was detected in the jet of 0954+658, providing evidence for the presence of a helical magnetic field surrounding the jet. For three of the sources…
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