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Record W3205825871 · doi:10.1093/mnras/stac883

The SN Ia runaway LP 398-9: detection of circumstellar material and surface rotation

2022· preprint· en· W3205825871 on OpenAlexafffund
Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska, Simon Blouin, Andrew Swan, T. R. Marsh, Ken J. Shen, B. T. Gänsicke, J. J. Hermes, Odelia Putterman, Evan B. Bauer, Evan Petrosky, S. P. Littlefair, R. P. Ashley

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsUniversity of Victoria
FundersH2020 European Research CouncilStockholms UniversitetUniversity of California, Los AngelesScience and Technology Facilities CouncilInstituto de Astrofísica de CanariasDeutsches Elektronen-SynchrotronLaboratory Directed Research and DevelopmentNational Science FoundationLiverpool John Moores UniversityJet Propulsion LaboratoryUniversity of MarylandCentre National d’Etudes SpatialesCalifornia Institute of TechnologyGovernment of CanadaLos Alamos National LaboratoryUniversity of WashingtonEuropean Space AgencyJohns Hopkins UniversitySpace Telescope Science InstituteMinistry of Science and TechnologyNational Aeronautics and Space AdministrationEuropean CommissionNuclear Safety and Security CommissionPlanetary Science DivisionInstitute for Advanced StudyHarvard UniversityUniversity of California
KeywordsSupernovaWhite dwarfPhysicsAstrophysicsThermonuclear fusionBrightnessRotation periodRotation (mathematics)AstronomyStarsPlasmaGeometry

Abstract

fetched live from OpenAlex

ABSTRACT A promising progenitor scenario for Type Ia supernovae (SNeIa) is the thermonuclear detonation of a white dwarf in a close binary system with another white dwarf. After the primary star explodes, the surviving donor can be spontaneously released as a hypervelocity runaway. One such runaway donor candidate is LP 398-9, whose orbital trajectory traces back ≈105 yr to a known supernova remnant. Here, we report the discovery of carbon-rich circumstellar material around LP 398-9, revealed by a strong infrared excess and analysed with follow-up spectroscopy. The circumstellar material is most plausibly composed of inflated layers from the star itself, mechanically and radioactively heated by the past companion’s supernova. We also detect a 15.4 h periodic signal in the UV and optical light curves of LP 398-9, which we interpret as surface rotation. The rotation rate is consistent with theoretical predictions from this supernova mechanism, and the brightness variations could originate from surface inhomogeneity deposited by the supernova itself. Our observations strengthen the case for this double-degenerate SNIa progenitor channel, and motivate the search for more runaway SNIa donors.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
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
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.007
GPT teacher head0.235
Teacher spread0.227 · 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

Citations1
Published2022
Admission routes2
Has abstractyes

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