AGN Jets and Winds in Polarised Light: The Case of Mrk 231
Silpa S. (NCRA-TIFR), P. Kharb (NCRA-TIFR), C. P. O' Dea (University, of Manitoba), S. A. Baum (University of Manitoba), B. Sebastian (Purdue, University), D. Mukherjee (IUCAA), C. M. Harrison (Newcastle University)

TL;DR
This study uses multi-frequency radio polarimetric observations to reveal a complex, magnetized outflow structure in Mrk 231, including a weakly collimated jet and surrounding wind, providing insights into AGN feedback mechanisms.
Contribution
It presents detailed polarimetric imaging of Mrk 231, demonstrating the presence of a broad, magnetized outflow with a jet and wind structure, and estimates the jet production efficiency.
Findings
Detection of a broad, curved outflow with a weakly collimated jet
Magnetic fields inferred as poloidal in the jet and toroidal in the wind
Jet production efficiency estimated at approximately 1%
Abstract
We present the results of a multi-frequency, multi-scale radio polarimetric study with the Very Large Array (VLA) of the Seyfert 1 galaxy and BALQSO, Mrk 231. We detect complex total and polarized intensity features in the source. Overall, the images indicate the presence of a broad, one-sided, curved outflow towards the south which consists of a weakly collimated jet with poloidal inferred magnetic fields, inside a broader magnetized ``wind'' or ``sheath'' component with toroidal inferred magnetic fields. The model of a kpc-scale weakly collimated jet/lobe in Mrk 231 is strengthened by its C-shaped morphology, steep spectral index throughout, complexities in the magnetic field structures, and the presence of self-similar structures observed on the 10-parsec-scale in the literature. The ``wind'' may comprise both nuclear starburst (close to the core) and AGN winds, where the latter…
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