# The polarized signal from broad emmission lines in AGN

## TL;DR

This study uses advanced radiative transfer simulations to analyze the spectropolarimetric signals from broad emission lines in AGN, revealing new insights into the geometry and kinematics of the scattering regions.

## Contribution

It demonstrates that thicker, more optically dense scatterers and outflows significantly influence the polarization signals, challenging previous models and providing new diagnostic tools.

## Key findings

- Thicker, optically dense scatterers reproduce polarization features.
- Outflows enhance the polarization angle signal.
- Distinct M-shaped PA profiles indicate cospatial, outflowing scatterers.

## Abstract

Using the STOKES Monte Carlo radiative transfer code we revisit the predictions of the spectropolarimetric signal from a disc-like Broad Emission Line Region (BLR) in Type I AGN due to equatorial scattering. We reproduce the findings of previous works, but only for a scatterer which is much more optically and geometrically thick than previously proposed. We also find that when taking into account the polarized emission from all regions of the scatterer, the swing of the Polarizarion Angle (PA) is in the opposite direction to that originally proposed. Furthermore, we find that the presence of outflows in the scattering media can significantly change the observed line profiles, with the PA of the scattering signal being enhanced in the presence of radially outflowing winds. Finally, a characteristically different PA profile, shaped like an `M', is seen when the scatterer is cospatial with the BLR and radially outflowing.