Parsec Scale Faraday-Rotation Structure Across the Jets of 9 Active Galactic Nuclei
arXiv:1709.09062 · doi:10.1093/mnras/stx2127
Abstract
A number of groups have recently been active in searching for gradients in the ob- served Faraday rotation measure (RM) across jets of Active Galactic Nuclei (AGNs) on various scales and estimating their reliability. Such RM structures provide direct evidence for the presence of an azimuthal magnetic field component, which may be associated with a helical jet magnetic field, as is expected based on the results of many theoretical studies. We present new parsec-scale RM maps of 4 AGNs here, and analyze their transverse RM structures together with those for 5 previously published RM maps. All these jets display transverse RM gradients with significances of at least 3σ. This is part of an ongoing effort to establish how common transverse RM gradients that may be associated with helical or toroidal magnetic fields are in AGNs on parsec scales.
11 pages, 4 figures, 3 tables
References in corpus (6)
- MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VIII. Faraday rotation in parsec-scale AGN 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
- The 15--43-GHz Parsec-scale Circular Polarization of 41 Active Galactic Nuclei
- High resolution VLBI polarisation imaging of AGN with the Maximum Entropy Method
- 18-22 cm VLBA Faraday rotation studies of six AGN jets
Cited by in corpus (7)
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- Synchrotron intensity plots from a relativistic stratified jet
- Radio VLBA polarization and multi-band monitoring of the high-redshift quasar S5 0836+710 during a high activity period
- Helical Magnetic Field in a Massive Protostellar Jet
- First Adiabatic Invariant and the Brightness Temperature of Relativistic Jets
- Depolarization and Faraday effects in AGN Jets