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Record W4200630188 · doi:10.1093/mnras/stab3662

ASAS J071404+7004.3 – a close, bright nova-like cataclysmic variable with gusty winds

2021· article· en· W4200630188 on OpenAlexfundno aff
Keith Inight, Dominic Blondel, D. Boyd, R. P. Ashley, C. Knigge, Knox S. Long, T. R. Marsh, J McCleery, Simone Scaringi, D. Steeghs, J. R. Thorstensen, Tonny Vanmunster, P. J. Wheatley

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersPlanetary Science DivisionScience and Technology Facilities CouncilScience Mission DirectorateSmithsonian Astrophysical ObservatoryUniversity of California, Los AngelesJet Propulsion LaboratoryUniversity of EdinburghMax-Planck-Institut für AstronomieUniversity of MarylandCentre National d’Etudes SpatialesInstituto de Astrofísica de CanariasNational Aeronautics and Space AdministrationUniversity College LondonQueen's UniversityUniversity of LeicesterSpace Telescope Science InstituteLos Alamos National LaboratoryGoddard Space Flight CenterEuropean Space AgencyJohns Hopkins UniversityAstrophysics Science DivisionGordon and Betty Moore FoundationQueen's University BelfastMinistry of Science and TechnologyNational Science FoundationAstrophysics DivisionDurham UniversitySmithsonian InstitutionEötvös Loránd TudományegyetemCalifornia Institute of TechnologyUniversity of Hawai'iNational Central UniversityLeverhulme Trust
KeywordsCataclysmic variable starPhysicsAstrophysicsPhotometry (optics)Light curveVariable starSwiftSpectroscopyAstronomyStarsWhite dwarf

Abstract

fetched live from OpenAlex

ABSTRACT Despite being bright (V ≃ 11.8) and nearby (d = 212 pc) ASAS J071404+7004.3 has only recently been identified as a nova-like cataclysmic variable. We present time-resolved optical spectroscopy obtained at the Isaac Newton and the Hiltner and McGraw-Hill Telescopes, together with Swift X-ray and ultraviolet observations. We combined these with TESS photometry and find a period of 3.28 h and a mass transfer rate of $4\!-\!9\times 10^{-9}\, {\mathrm{M_{\odot }\, yr}^{-1}}$. Historical photometry shows at least one low state establishing the system as a VY Scl star. Our high-cadence spectroscopy also revealed rapidly changing winds emanating from the accretion disc. We have modelled these using the Monte Carlo python code and shown that all the emission lines could emanate from the wind – which would explain the lack of double-peaked lines in such systems. In passing, we discuss the effect of variability on the position of cataclysmic variables in the Gaia Hertzsprung–Russell diagram.

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 score0.005
Threshold uncertainty score0.012

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)0.0040.001

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 head0.008
GPT teacher head0.197
Teacher spread0.189 · 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 routes1
Has abstractyes

Explore more

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