MétaCan
Menu
Back to cohort
Record W4410259103 · doi:10.1093/mnrasl/slaf047

Is the symbiotic recurrent nova T CrB late? Recent photometric evolution and comparison with past pre-outburst behaviour

2025· article· en· W4410259103 on OpenAlexaff
Jaroslav Merc, Ł. Wyrzykowski, P. G. Beck, P. Mikołajczyk, Krzysztof Kotysz, Paweł Zieliński, S. Zoła, Sebastian Kurowski, W. Ogłoza, M. Dróżdż, Charles Galdies, Franz-Josef Hambsch, Stephen M. Brincat, B. Joachimczyk, M. Bronikowski, Jure Japelj, J. M. Carrasco, U. Burgaz, A. Gurgul, K. Bąkowska, Piotr Hofbauer, K. Szyszka, J. Golonka, J. K. T. Qvam, J. Zdanavičius, E. Pakštienė, M. Maskoliūnas, Vytautas Čepas, Uliana Pylypenko, D. Moździerski, Franky Dubois, S. Vanaverbeke, J. M. Olszewska, A. Liakos, M. Stojanović, G. Damljanović, Adam Popowicz, Mateusz Marzec, Magdalena Badura, Alicja Pucek, Mateusz Szklarz, T. Kvernadze, A. Reguitti, Supachai Awiphan, M. Dennefeld, K. Gazeas

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society Letters · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsTrinity College
FundersInstitut de Ciències del CosmosAgencia Estatal de InvestigaciónHORIZON EUROPE Framework ProgrammeUniwersytet Mikolaja Kopernika w ToruniuLietuvos Mokslo TarybaIntegrated Electronics Engineering Center, Binghamton UniversityGrantová Agentura České RepublikyJavna Agencija za Raziskovalno Dejavnost RSEuropean Regional Development FundEuropean CommissionMinisterio de Ciencia e InnovaciónNarodowe Centrum NaukiEuropean Space AgencyThailand Science Research and InnovationUniversitat de BarcelonaFP7 Research Potential of Convergence RegionsNational Astronomical Research Institute of Thailand
KeywordsPhysicsNova (rocket)AstrophysicsAstronomy

Abstract

fetched live from OpenAlex

ABSTRACT T CrB is a symbiotic recurrent nova that last erupted in 1946. Given its recurrence time-scale of approximately 80 yr, the next outburst is eagerly anticipated by the astronomical community. In this work, we analyse the optical light curves of T CrB, comparing recent photometric evolution with historical data to evaluate potential predictive indicators of nova eruptions. Although the ‘superactive’ phases preceding both the 1946 and anticipated eruptions are strikingly similar, the subsequent photometric behaviour differs. We find that the decline in brightness observed in 2023, interpreted by some as a ‘pre-eruption dip’, deviates from the deep minimum recorded prior to the 1946 event and does not reliably predict the eruption timing. Recent photometric and spectroscopic observations indicate that the system is returning to a high-accretion state. Given this, an eruption may be imminent, even without distinct precursors. While the next eruption of T CrB will be a major scientific event, its expected peak brightness of $V \sim 2$ mag highlights the importance of setting realistic public expectations for what will be a visually modest, yet astrophysically very significant, celestial event.

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)0.001
metaresearch head score (Gemma)0.002
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 score0.010
Threshold uncertainty score0.020

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
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 head0.228
Teacher spread0.218 · 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".

Quick stats

Citations8
Published2025
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society LettersSame topicGamma-ray bursts and supernovaeFrench-language works237,207