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Record W4390392980 · doi:10.1093/mnrasl/slad195

The metamorphosis of the Type Ib SN 2019yvr: late-time interaction

2023· article· en· W4390392980 on OpenAlexfundno aff
Lucía Ferrari, G. Folatelli, H. Kuncarayakti, M. Stritzinger, Keiichi Maeda, Melina C. Bersten, M. M. Saez, Luc Dessart, Peter Lundqvist, P. A. Mazzali, T. Nagao, C. Ashall, S. Bose, S. Brennan, Yongzhi Cai, R. Handberg, S. Holmbo, E. Karamehmetoglu, A. Pastorello, A. Reguitti, J. P. Anderson, T. W. Chen, L. Galbany, M. Gromadzki, C. P. Gutiérrez, C. Inserra, E. Kankare, T. E. Müller-Bravo, S. Mattila, M. Nicholl, G. Pignata, J. Sollerman, Shubham Srivastav, D. R. Young

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society Letters · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersConsejo Superior de Investigaciones CientíficasJapan Society for the Promotion of ScienceEuropean Social FundAgencia Nacional de Investigación y DesarrolloH2020 European Research CouncilStockholms UniversitetTurun YliopistoAgencia Estatal de InvestigaciónUniversitetet i OsloInfocomm Development Authority of SingaporeGeneralitat de CatalunyaMinisterio de Ciencia e InnovaciónDanmarks Frie ForskningsfondHáskóli ÍslandsNational Natural Science Foundation of ChinaScience and Technology Facilities CouncilEsperantic Studies FoundationOpetushallitusEuropean CommissionAarhus UniversitetInstitut sur la Nutrition et les Aliments FonctionnelsAlbert Ellis Institute
KeywordsPhysicsAstrophysicsEjectaSupernovaLight curveRADIUSLuminosityLine (geometry)Emission spectrumH-alphaType (biology)Spectral lineType II supernovaStar (game theory)AstronomyGalaxyGeometry

Abstract

fetched live from OpenAlex

ABSTRACT We present observational evidence of late-time interaction between the ejecta of the hydrogen-poor Type Ib supernova (SN) 2019yvr and hydrogen-rich circumstellar material (CSM), similar to the Type Ib SN 2014C. A narrow H α emission line appears simultaneously with a break in the light-curve decline rate at around 80–100 d after explosion. From the interaction delay and the ejecta velocity, under the assumption that the CSM is detached from the progenitor, we estimate the CSM inner radius to be located at ∼6.5–9.1 × 1015 cm. The H α emission line persists throughout the nebular phase at least up to +420 d post-explosion, with a full width at half maximum of ∼2000 km s−1. Assuming a steady mass-loss, the estimated mass-loss rate from the luminosity of the H α line is ∼3–7 × 10−5 M⊙ yr−1. From hydrodynamical modelling and analysis of the nebular spectra, we find a progenitor He-core mass of 3–4 M⊙, which would imply an initial mass of 13–15 M⊙. Our result supports the case of a relatively low-mass progenitor possibly in a binary system as opposed to a higher mass single star undergoing a luminous blue variable phase.

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 score0.003
Threshold uncertainty score0.006

Distilled classifier scores by category (both heads)

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 communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.207
Teacher spread0.199 · 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

Citations9
Published2023
Admission routes1
Has abstractyes

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