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A new Bowen fluorescence flare and extreme coronal line emitter discovered by SRG/eROSITA

2025· article· en· W7124176977 on OpenAlexfundno aff
P. Baldini, A. Rau, R. Arcodia, T. Ryu, Z. Liu, P. Sánchez-Sáez, I. Grotova, A. Merloni, S. Ciroi, A. J. Goodwin, M. Gromadzki, A. Kawka, M. Masterson, D. Tubín-Arenas, D. A. H. Buckley, F. Di Mille, G. E. Anderson, S. Bahic, D. Homan, M. Krumpe, J. C. A. Miller-Jones, K. Nandra

Bibliographic record

VenueSpringer Link (Chiba Institute of Technology) · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersScience and Technology Facilities CouncilRheinische Friedrich-Wilhelms-Universität BonnChinese Academy of SciencesQueen's UniversityEberhard Karls Universität TübingenLeibniz-Institut für Astrophysik PotsdamNational Aeronautics and Space AdministrationRussian Academy of SciencesCommonwealth Scientific and Industrial Research OrganisationQueen's University BelfastLeibniz-GemeinschaftCentre National d’Etudes SpatialesAustralian GovernmentUniversität HamburgMax-Planck-GesellschaftSpace Telescope Science Institute
KeywordsBalmer seriesFlareEmission spectrumAccretion (finance)Light curveRedshiftLine (geometry)Supermassive black hole

Abstract

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The nuclear X-ray transient eRASSt J012026.5−292727 (J012026 hereafter) was discovered in the second SRG/eROSITA all-sky survey (eRASS2). The source appeared more than one order of magnitude brighter than the eRASS1 upper limits (peak eRASS2 0.2–2.3 keV flux of 1.14 × 10−12 erg cm−2 s−1) and with a soft X-ray spectrum (photon index of Γ = 4.3). Over the following months, the X-ray flux started decaying and demonstrated significant flaring activity on both short (hour) and long (year) timescales. By inspecting the multiwavelength light curves of time-domain wide-field facilities, we detected a strong mid-infrared flare, which evolved over two years, and a weaker optical counterpart, with possible hints of a rise > 3 years prior to the X-ray discovery. Follow-up optical spectroscopy revealed transient features, including redshifted Balmer lines (FWHM of ∼1500 km s−1), strong Fe II emission, He II, Bowen fluorescence lines, and high-ionization coronal lines such as [Fe X] and [Fe XIV]. One spectrum displayed a triple-peaked Hβ line, consistent with emission from a face-on elliptical accretion disk. The spectroscopic features and the slow evolution of the event place J012026 within the nuclear-transient classifications of Bowen fluorescence flares (BFFs) and extreme coronal line emitters (ECLEs). BFFs have been associated with rejuvenated accreting supermassive black holes, although the mechanism triggering the onset of the new accretion flow is yet to be understood, while ECLEs have been linked to the disruption and accretion of stars in gas-rich environments. The association of J012026 with both classes, combined with the X-ray, multiwavelength, and spectroscopic information, supports the idea that the BFF emission could be, at least in some cases, triggered by tidal disruption events (TDEs) perturbing gaseous environments. The observed short- and long-term X-ray variability, uncommon in standard TDEs, adds complexity to these families of nuclear transients. These results highlight the diverse phenomenology of nuclear accretion events and demonstrate the value of systematic X-ray surveys, such as eROSITA and Einstein Probe, for uncovering such transients and characterizing their physical origin.

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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 score0.002
Threshold uncertainty score0.004

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 communication0.0010.000
Open science0.0000.001
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 head0.011
GPT teacher head0.226
Teacher spread0.214 · 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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