A1 Refereed original research article in a scientific journal
Optical polarization properties of the closest tidal disruption event AT 2023clx indicate origin from tidal stream shocks
Authors: Koljonen, Karri I. I.; Nilsson, Kari; Liodakis, Ioannis; Lindfors, Elina
Publisher: Oxford University Press (OUP)
Publication year: 2025
Journal:: Monthly Notices of the Royal Astronomical Society
Volume: 542
Issue: 3
First page : 2238
Last page: 2244
ISSN: 0035-8711
eISSN: 1365-2966
DOI: https://doi.org/10.1093/mnras/staf1340
Web address : https://doi.org/10.1093/mnras/staf1340
Self-archived copy’s web address: https://research.utu.fi/converis/portal/detail/Publication/500280952
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 similar to 5 per cent. In addition, the polarization angle shifts by similar to 60 degrees-100 degrees between 6 and 20 d 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 disc 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 disc formation.
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Funding information in the publication:
We sincerely thank Panagiotis Charalampopoulos for providing the NOT V-band polarization data (obtained under programme P66-019) and the host-subtracted spectra taken close to our NOT observations. We also thank the anonymous referee for comments that improved the manuscript.
