Scattered synchrotron emission and a giant torus revealed in polarized light in the nearest radio galaxy Centaurus A

TL;DR

This study uses optical and near-infrared spectropolarimetry to reveal a giant torus and scattered synchrotron emission in Centaurus A, providing insights into its nuclear structure and emission mechanisms.

Contribution

It demonstrates that a beamed synchrotron jet scattering onto the narrow line region explains the polarized emission and nuclear geometry in Centaurus A, revealing a hidden NLR AGN structure.

Findings

Polarized emission shows a polarization degree of 2-4%.

The polarization angle is perpendicular to the radio jet axis.

Evidence supports a beamed synchrotron jet scattering model.

Abstract

Centaurus A (Cen A) is the closest radio galaxy and a prime example of a low-luminosity active galactic nucleus (AGN), exhibiting complex emissions across the electromagnetic spectrum. The nature of its continuum emission, particularly the mechanisms powering it, has been a subject of considerable debate due to the fact that the AGN is deeply buried in dust. This study aims to elucidate the origin of the continuum emission in Cen A and determine the geometrical arrangement of matter in the nuclear region by the mean of optical and near-infrared spectropolarimetry. We obtained spectropolarimetric data of Cen A using the VLT/FORS2. The analysis revealed a region showing strong and narrow emission lines associated with AGN activity. After correction for interstellar polarization in the dust lane (but not for starlight), the intrinsic polarization of the scattered AGN light exhibits a polarization degree of 2-4%, decreasing from optical to near-infrared, associated with a polarization position angle perpendicular to the radio jet axis. We exclude the presence of hidden broad line in our polarized flux spectrum at more than 99% probability. Narrow emission lines are found to be strongly polarized and orthogonal to the jet position angle. We demonstrate that a beamed synchrotron jet, scattering onto the narrow line region (NLR) best fits all the observational properties reported in this paper and the literature. In this model, the base of the NLR is obscured by a giant circumnuclear region and can only become visible through perpendicular scattering onto the outermost part of the NLR, naturally producing high polarization degrees and polarization angles perpendicular to the radio structure. This study provides strong evidence that Cen A defines a new class of hidden-NLR AGNs and supports old predictions that beamed synchrotron jets can be observed in reflection.