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Record W3198131901 · doi:10.3847/1538-4357/ac2237

Discovery of a 310 Day Period from the Enshrouded Massive System NaSt1 (WR 122)

2021· preprint· en· W3198131901 on OpenAlexafffund
Ryan M. Lau, Samaporn Tinyanont, M. Hankins, M. C. B. Ashley, Kishalay De, A. V. Filippenko, Lynne A. Hillenbrand, M. M. Kasliwal, Jon C. Mauerhan, A. F. J. Moffat, Anna Moore, Nathan Smith, Jamie Soon, Roberto Soria, Tony Travouillon, K. A. van der Hucht, P. M. Williams, WeiKang Zheng

Bibliographic record

VenueThe Astrophysical Journal · 2021
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsUniversité de MontréalCentre for Research in Astrophysics of Québec
FundersNatural Sciences and Engineering Research Council of CanadaDeutsches Elektronen-SynchrotronCenter for Cosmology and Astroparticle Physics, Ohio State UniversityStockholms UniversitetChinese Academy of SciencesUniversity of New South WalesScience and Technology Facilities CouncilWeizmann Institute of ScienceChinese Academy of Sciences South America Center for AstronomyAustralian GovernmentVillum FondenSpace Telescope Science InstituteNational Science FoundationUniversity of WashingtonNational Aeronautics and Space AdministrationJapan Aerospace Exploration AgencyCalifornia Institute of TechnologyOhio State UniversityAdolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California BerkeleyNuclear Safety and Security CommissionGordon and Betty Moore Foundation
KeywordsLight curvePhysicsAstrophysicsAstronomyOrbital periodAmplitudeSupernovaPhotometry (optics)WavelengthAsteroidInfraredStarsOptics

Abstract

fetched live from OpenAlex

Abstract We present optical and infrared (IR) light curves of NaSt1, also known as Wolf–Rayet 122, with observations from Palomar Gattini-IR (PGIR), the Zwicky Transient Facility (ZTF), the Katzman Automatic Imaging Telescope, the Asteroid Terrestrial-impact Last Alert System, and the All-Sky Automated Survey for Supernovae (ASAS-SN). We identify a P = 309.7 ± 0.7 day photometric period from the optical and IR light curves that reveal periodic, sinusoidal variability between 2014 July and 2021 July. We also present historical IR light curves taken between 1983 July and 1989 May, which show variability consistent with the period of the present-day light curves. In the past, NaSt1 was brighter in the J band with larger variability amplitudes than the present-day PGIR values, suggesting that NaSt1 exhibits variability on longer (≳decade) timescales. Sinusoidal fits to the recent optical and IR light curves show that the amplitude of NaSt1's variability differs at various wavelengths and also reveal significant phase offsets of 17.0 ± 2.5 day between the ZTF r and PGIR J light curves. We interpret the 310 day photometric period from NaSt1 as the orbital period of an enshrouded massive binary. We suggest that the photometric variability of NaSt1 may arise from variations in the line-of-sight optical depth toward circumstellar optical/IR-emitting regions throughout its orbit due to colliding-wind dust formation. We speculate that past mass transfer in NaSt1 may have been triggered by Roche-lobe overflow (RLOF) during an eruptive phase of an Ofpe/WN9 star. Lastly, we argue that NaSt1 is no longer undergoing RLOF mass transfer.

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 score0.002
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
Bibliometrics0.0010.001
Science and technology studies0.0010.000
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 head0.222
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 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

Citations0
Published2021
Admission routes2
Has abstractyes

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