The Structure & Linear Polarization of the Kiloparsec-Scale Jet of the Quasar 3C\,345
David H. Roberts, John F. C. Wardle, and Valerie V. Marchenko

TL;DR
This study uses deep radio imaging to analyze the structure and polarization of the 3C 345 quasar's jet, revealing a complex magnetic field configuration and jet dynamics on kiloparsec scales.
Contribution
It provides detailed measurements of the jet's polarization, structure, and magnetic field orientation, and suggests jet re-direction and helical magnetic fields as key features.
Findings
Jet length approximately 27 kpc.
Polarization pattern indicates a helical magnetic field.
Jet speed constrained to be greater than 0.5c.
Abstract
Deep Very Large Array imaging of the quasar 3C\,345 at 4.86 and 8.44 GHz has been used to study the structure and linear polarization of its radio jet on scales ranging from 2 to 30 kpc. There is a 7--8 Jy unresolved core with spectral index (). The jet (typical intensity 15 mJy/beam) consists of a straight section containing two knots, and two additional non-co-linear knots at the end. The jet's total projected length is about 27 kpc. The spectral index of the jet varies over . The jet diverges with a semi-opening angle of about , and is nearly constant in integrated brightness over its length. A faint feature north-east of the core does not appear to be a true counter-jet, but rather an extended lobe of this FR-II radio source seen in projection. The absence of a counter-jet is…
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