18-22 cm VLBA Faraday rotation studies of six AGN jets
arXiv:1702.06659 · doi:10.1093/mnras/stx256
Abstract
The formation of relativistic jets in active galactic nuclei (AGN) is related to accretion on to their central supermassive black holes, and magnetic fields are believed to play a central role in launching, collimating and accelerating the jet streams from very compact regions out to kiloparsec or megaparsec scales. In the presence of helical or toroidal magnetic fields threading the AGN jets and their immediate vicinity, gradients in the observed Faraday rotation measures are expected due to the systematic change in the line-of-sight component of the magnetic field across the jet. We have analysed total intensity, linear polarization, fractional polarization and Faraday rotation maps based on Very Long Baseline Array data obtained at four wavelengths in the 18-22 cm range for six AGN (OJ 287, 3C 279, PKS 1510-089, 3C 345, BL Lac and 3C 454.3). These observations typically probe projected distances out to tens of parsecs from the observed core, and are well suited for Faraday rotation studies due to the relatively long wavelengths used and the similarity of the structures measured at the different wavelengths. We have identified statistically significant, monotonic, transverse Faraday rotation gradients across the jets of four of these six sources, as well as a tentative transverse Faraday rotation gradient across the jet of OJ 287, providing evidence for the presence of toroidal magnetic fields, which may be one component of helical magnetic fields associated with these AGN jets.
arXiv comment17 pages, 9 figures, 5 tables. Accepted for publication in MNRAS Main Journal
References in corpus (25)
- MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VI. Kinematics Analysis of a Complete Sample of Blazar Jets
- MOJAVE: Monitoring of Jets in AGN with VLBA Experiments. V. Multi-epoch VLBA Images
- Stability of Relativistic Jets from Rotating, Accreting Black Holes via Fully Three-Dimensional Magnetohydrodynamic Simulations
- MOJAVE: Monitoring of Jets in AGN with VLBA Experiments - I. First-Epoch 15 GHz Linear Polarization Images
- Polarization and structure of relativistic parsec-scale AGN jets
- MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VIII. Faraday rotation in parsec-scale AGN jets
- A Helical Magnetic Field in the Jet of 3C 273
- Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron. I. Imaging BL Lacertae at 21 microarcsecond resolution
- A View through Faraday's Fog 2: Parsec Scale Rotation Measures in 40 AGN
- Radio Jet-Ambient Medium Interactions on Parsec Scales in the Blazar 1055+018
- Three dimensional magnetic field structure of six parsec-scale active galactic nuclei jets
- Parsec-scale Faraday Rotation Measures from General Relativistic MHD Simulations of Active Galactic Nuclei Jets
- A View through Faraday's fog: Parsec scale rotation measures in AGN
- Faraday Rotation Measure Gradients from a Helical Magnetic Field in 3C 273
- Parsec-Scale Blazar Monitoring: Flux and Polarization Variability
- Parsec-scale jet precession in BL Lacertae (2200+420)
- Precession in the inner jet of 3C 345
- 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
- Connecting Magnetic Towers with Faraday Rotation Gradients in Active Galactic Nuclei Jets
- Surprising Evolution of the Parsec-scale Faraday Rotation Gradients in the Jet of the BL Lac Object B1803+784
- Analysing the Transverse Structure of the Relativistic Jets of AGN
- Dominance of outflowing electric currents on decaparsec to kiloparsec scales in extragalactic jets
- High Frequency VLBI Rotation Measure of 8 AGN
- Modeling very long baseline interferometric images with the cross-entropy global optimization technique
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- Parsec Scale Faraday-Rotation Structure Across the Jets of 9 Active Galactic Nuclei
- The Jets of AGN as giant co-axial cables
- Reversals in the Direction of Polarization Rotation in OJ 287
- Blazar jet evolution revealed by multi-epoch broadband radio polarimetry
- Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron IV. The quasar 3C 345 at 18 cm: Magnetic field structure and brightness temperature
- Observational signatures of magnetic field structure in relativistic AGN jets
- Unveiling the Bent Jet Structure and Polarization of OJ 287 at 1.7 GHz with Space VLBI