Spectropolarimetry of High Redshift Obscured and Red Quasars

TL;DR

This study uses spectropolarimetry to explore the inner geometry and outflows of high-redshift obscured and red quasars, revealing dust scattering, polarization features, and outflow dynamics that support unification models.

Contribution

It presents the first optical spectropolarimetric observations of high-redshift obscured quasars, proposing a dust scattering model with outflows that explains polarization features and inner region geometry.

Findings

Polarization fractions >10% in some quasars

Detection of 90-degree polarization angle swings

Evidence for dusty outflows and toroidal obscuration

Abstract

Spectropolarimetry is a powerful technique that has provided critical support for the geometric unification model of local active galactic nuclei. In this paper, we present optical (rest-frame UV) Keck spectropolarimetry of five luminous obscured (Type 2) and extremely red quasars (ERQs) at z~2.5. Three objects reach polarization fractions of >10% in the continuum. We propose a model in which dust scattering is the dominant scattering and polarization mechanism in our targets, though electron scattering cannot be completely excluded. Emission lines are polarized at a lower level than is the continuum. This suggests that the emission-line region exists on similar spatial scales as the scattering region. In three objects we detect an intriguing 90 degree swing in the polarization position angle as a function of line-of-sight velocity in the emission lines of Ly-alpha, CIV and NV. We interpret this phenomenon in the framework of a geometric model with an equatorial dusty scattering region in which the material is outflowing at several thousand km/sec. Emission lines may also be scattered by dust or resonantly. This model explains several salient features of observations by scattering on scales of a few tens of pc. Our observations provide a tantalizing view of the inner region geometry and kinematics of high-redshift obscured and extremely red quasars. Our data and modeling lend strong support for toroidal obscuration and powerful outflows on the scales of the UV emission-line region, in addition to the larger scale outflows inferred previously from the optical emission-line kinematics.