Estimations of the magnetic field strength in the torus of AGN using near-infrared polarimetry

TL;DR

This study estimates the magnetic field strength in the torus of AGN IC5063 using near-infrared polarimetry, modeling dust grain alignment and applying the Chandrasekhar-Fermi method to understand magnetic influence on the torus structure.

Contribution

The paper introduces a polarisation model to estimate magnetic field strength in AGN tori using near-infrared polarimetry and dust grain alignment mechanisms, providing new insights into magnetic roles in AGN environments.

Findings

Magnetic field strength in the torus of IC5063 is estimated to be between 12-128 mG.

The polarisation is consistent with dichroic absorption by aligned dust grains.

The study demonstrates the feasibility of using polarimetry to probe magnetic fields in AGN tori.

Abstract

An optically and geometrically thick torus obscures the central engine of Active Galactic Nuclei (AGN) from some lines of sight. From a magnetohydrodynamical framework, the torus can be considered to be a particular region of clouds surrounding the central engine where the clouds are dusty and optically thick. In this framework, the magnetic field plays an important role in the creation, morphology and evolution of the torus. If the dust grains within the clouds are assumed to be aligned by paramagnetic alignment, then the ratio of the intrinsic polarisation and visual extinction, P(%)/Av, is a function of the magnetic field strength. To estimate the visual extinction through the torus and constrain the polarisation mechanisms in the nucleus of AGN, we developed a polarisation model to fit both the total and polarised flux in a 1.2" (~263pc) aperture of the type 2 AGN, IC5063. The polarisation model is consistent with the nuclear polarisation observed at K being produced by dichroic absorption from aligned dust grains with a visual extinction through the torus of 48$\pm$2 mag. We estimated the intrinsic polarisation arising from dichroic absorption to be P$_{K}^{dic}$=12.5$\pm$2.7%. We consider the physical conditions and environment of the gas and dust for the torus of IC5063. Then, through paramagnetic alignment, we estimate a magnetic field strength in the range of 12-128mG in the NIR emitting regions of the torus of IC5063. Alternatively, we estimate the magnetic field strength in the plane of the sky using the Chandrasekhar-Fermi method. The minimum magnetic field strength in the plane of the sky is estimated to be 13 and 41 mG depending of the conditions within the torus of IC5063. These techniques afford the chance to make a survey of AGN, to investigate the effects of magnetic field strength on the torus, accretion, and interaction to the host galaxy.