Optical polarization properties of the closest tidal disruption event AT 2023clx indicate origin from tidal stream shocks

TL;DR

This study presents optical polarization observations of the tidal disruption event AT 2023clx, revealing polarization variability consistent with tidal stream shocks driving the optical outburst during accretion disk formation.

Contribution

First polarization measurements of AT 2023clx showing variability linked to tidal stream shocks, providing new insights into accretion processes in tidal disruption events.

Findings

Polarization degree peaked at ~5% and varied over time.

Polarization angle shifted by 60-100 degrees post-peak.

Variability pattern similar to AT 2020mot, indicating a common mechanism.

Abstract

Polarization observations of tidal disruption events offer unique insights into the accretion processes around supermassive black holes. Here, we present optical polarization observations of the nearby event AT 2023clx, obtained using the Nordic Optical Telescope. Our observations reveal a rise and subsequent decay in the polarization degree, temporally offset from the peak of the optical light curve, reaching maximum intrinsic polarization degree of $\sim$5 per cent. In addition, the polarization angle shifts by $\sim60^\circ-100^\circ$ between 6 to 20 days after the optical peak, remaining stable thereafter. Remarkably, the observed polarization variability closely resembles that of AT 2020mot, strongly suggesting a common mechanism for accretion disk formation in these events. The variability in both polarization degree and angle supports models in which tidal stream shocks drive the optical outburst during the accretion disk formation.