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Optical polarisation of stellar-fed active and quiescent supermassive black holes

2025· article· en· W7114785710 on OpenAlexfundno aff

Bibliographic record

VenueSpringer Link (Chiba Institute of Technology) · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilStockholms UniversitetDeutsches Elektronen-SynchrotronLiverpool John Moores UniversityTrinity College DublinQueen's UniversityCalifornia Institute of TechnologyEuropean CommissionQueen's University BelfastNational Aeronautics and Space AdministrationAlexander von Humboldt-StiftungDeutsche ForschungsgemeinschaftSpace Telescope Science InstituteNational Science Foundation
KeywordsSupermassive black holePolarimeterActive galactic nucleusLight curvePolarimetryFlarePolarization (electrochemistry)Broadband

Abstract

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Context. The advent of wide-field optical surveys with multi-wavelength capabilities has been a breakthrough in the detection and characterisation of bright, long-lasting optical flares from supermassive black holes, such as tidal disruption events (TDEs), Bowen flares in active galactic nuclei (AGNs), and changing-look AGNs. Yet, the physical mechanisms powering these diverse transient events remain highly debated. Aims. We aim to provide novel model constraints by utilising broadband optical polarimetry to study five TDEs. Our goal is to enhance the understanding of the reprocessing material involved in TDEs and to compare our findings with similar flaring activity observed in AGNs. Methods. Using the MOPTOP polarimeter on the 2 metre Liverpool Telescope, we conducted a monitoring campaign targeting three optically discovered TDEs (AT2024bgz, AT2024pvu, and AT2024wsd) and two Bowen flares in AGNs (AT2020afhd and AT2019aalc). Results. The three thermal TDEs show low intrinsic polarisation levels (ΔP ≈ 0 − 6%) with stable polarisation angles. The Bowen flares also show variable polarisation degrees (ΔP ≈ 0 − 8%) but significant polarisation angle variability: AT2020afhd exhibited a Δθ = 83 ± 8° shift at 150 days post-optical peak, while the AT2019aalc displayed quasi-periodic swings of Δθ ≈ 40° amplitude starting 190 days after peak brightness. Conclusions. The TDEs of this study are well described by models invoking rapid disk formation and reprocessed emission from optically thick outflows, whereas the Bowen flares reveal more complex reprocessing geometries, potentially consistent with TDEs occurring in AGN gas-rich environments. We find that moderate polarisation is observed at later times for TDEs with low-Eddington ratios and highly extended photospheres. This implies that, as the accretion level declines, we expect more asymmetric reprocessing layers along a given viewing angle. Since the outflow density and velocity depend sensitively on the inclination angle, we expect TDEs with low-Eddington ratios and highly extended photospheres to exhibit varying levels of polarisation. The polarisation of AT2019aalc (Seyfert 1) hints at a clumpy, asymmetric outflow and the presence of a tilted, precessing accretion disk, while the polarisation of AT2020afhd (AGN type 2) is consistent with the detection of a scattered light echo.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.010
GPT teacher head0.233
Teacher spread0.224 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations0
Published2025
Admission routes1
Has abstractyes

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