On the source of Faraday rotation in the jet of the radio galaxy 3C120
Jos\'e L. G\'omez, Mar Roca-Sogorb, Iv\'an Agudo, Alan P. Marscher,, Svetlana G. Jorstad

TL;DR
This study investigates the Faraday rotation in the jet of radio galaxy 3C120 using VLBA observations over several years, revealing complex, uncorrelated changes that suggest multiple Faraday rotation sources and a sheath of thermal electrons.
Contribution
It provides new insights into the origin of Faraday rotation in 3C120's jet, distinguishing between a sheath and foreground clouds as contributing factors.
Findings
RM remains constant at 2-5 mas from the core
Sign reversals in RM indicate localized Faraday rotation regions
RM-corrected EVPAs are perpendicular to the jet axis
Abstract
The source of Faraday rotation in the jet of the radio galaxy 3C120 is analyzed through Very Long Baseline Array observations carried out between 1999 and 2007 at 86, 43, 22, 15, 12, 8, 5, 2, and 1.7 GHz. Comparison of observations from 1999 to 2001 reveals uncorrelated changes in the linear polarization of the underlying jet emission and the Faraday rotation screen: while the rotation measure (RM) remains constant between approximately 2 and 5 mas from the core, the RM-corrected electric vector position angles (EVPAs) of two superluminal components are rotated by almost 90 degrees when compared to other components moving through similar jet locations. On the other hand, the innermost 2 mas experiences a significant change in RM -- including a sign reversal -- but without variations in the RM-corrected EVPAs. Similarly, observations in 2007 reveal a double sign reversal in RM along the…
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