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Record W4408372213 · doi:10.1038/s41550-025-02491-0

Sporadic radio pulses from a white dwarf binary at the orbital period

2025· article· en· W4408372213 on OpenAlexafffund
Iris de Ruiter, Kaustubh Rajwade, C. Bassa, A. Rowlinson, R. A. M. J. Wijers, C. D. Kilpatrick, Guðmundur Stefánsson, J. R. Callingham, J. W. T. Hessels, T. Clarke, Wendy Peters, R. Wijnands, T. W. Shimwell, S. ter Veen, V. Morello, Gregory R. Zeimann, Suvrath Mahadevan

Bibliographic record

VenueNature Astronomy · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsMcGill University
FundersU.S. Naval Research LaboratoryScience and Technology Facilities CouncilLeibniz-GemeinschaftObservatoire de Paris, Université de Recherche Paris Sciences et LettresMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenOffice of Naval ResearchCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftCanada Excellence Research Chairs, Government of CanadaNederlandse Organisatie voor Wetenschappelijk OnderzoekBundesministerium für Bildung und ForschungUniversiteit van AmsterdamScience Foundation IrelandEuropean CommissionUniversity of LeicesterLeibniz-Institut für Astrophysik PotsdamUniversité d'OrléansNational Aeronautics and Space AdministrationEuropean Space AgencyMcGill University
KeywordsWhite dwarfOrbital periodPeriod (music)White (mutation)AstronomyBinary numberAstrophysicsPhysicsBiologyMathematicsGeneticsAcousticsStars

Abstract

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Abstract Recent observations have revealed rare, previously unknown flashes of cosmic radio waves lasting from milliseconds to minutes, with a periodicity of minutes to an hour. These transient radio signals must originate from sources in the Milky Way and from coherent emission processes in astrophysical plasma. They are theorized to be produced in the extreme and highly magnetized environments around white dwarfs or neutron stars. However, the astrophysical origin of these signals remains contested, and multiple progenitor models may be needed to explain their diverse properties. Here we present the discovery of a transient radio source, ILT J1101 + 5521, whose roughly minute-long pulses arrive with a periodicity of 125.5 min. We find that ILT J1101 + 5521 is an M dwarf–white dwarf binary system with an orbital period that matches the period of the radio pulses, which are observed when the two stars are in conjunction. The binary nature of ILT J1101 + 5521 establishes that some long-period radio transients originate from orbital motion modulating the observed emission, as opposed to an isolated rotating star. We conclude that ILT J1101 + 5521 is probably a polar system where magnetic interaction has synchronized the rotational and orbital periods of the white dwarf. Magnetic interaction and plasma exchange between two stars has been theorized to generate sporadic radio emission, making ILT J1101 + 5521 a potential low-mass analogue to such mechanisms.

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How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.239
Threshold uncertainty score0.999

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0020.000

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 head0.004
GPT teacher head0.215
Teacher spread0.211 · 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 teacher head, not a consensus.

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

Citations35
Published2025
Admission routes2
Has abstractyes

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