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Record W2965920425 · doi:10.1051/0004-6361/201935511

The evolution of luminous red nova AT 2017jfs in NGC 4470

2019· article· en· W2965920425 on OpenAlexfundno aff

Bibliographic record

VenueAstronomy and Astrophysics · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersPlanetary Science DivisionRussian Academy of SciencesScience Mission DirectorateScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeSmithsonian Astrophysical ObservatoryInstituto de Astrofísica de CanariasEötvös Loránd TudományegyetemLomonosov Moscow State UniversityMax-Planck-GesellschaftChinese Academy of SciencesNational Science FoundationScience Foundation IrelandLiverpool John Moores UniversitySmithsonian InstitutionNational Natural Science Foundation of ChinaSpace Telescope Science InstituteCenter for Cosmology and Astroparticle Physics, Ohio State UniversityNational Central UniversityVillum FondenMinisterio de Ciencia e InnovaciónMax-Planck-Institut für AstronomieUniversity of EdinburghJohns Hopkins UniversityQueen's UniversityOhio State UniversityGordon and Betty Moore FoundationQueen's University BelfastChina Scholarship CouncilNational Aeronautics and Space AdministrationChinese Academy of Sciences South America Center for AstronomyDurham University
KeywordsLight curveLuminosityAbsolute magnitudeEmission spectrumRed giantSolar massWavelengthLuminous intensityEnvelope (radar)

Abstract

fetched live from OpenAlex

We present the results of our photometric and spectroscopic follow-up of the intermediate-luminosity optical transient AT 2017jfs . At peak, the object reaches an absolute magnitude of M g = −15.46 ± 0.15 mag and a bolometric luminosity of 5.5 × 10 41 erg s −1 . Its light curve has the double-peak shape typical of luminous red novae (LRNe), with a narrow first peak bright in the blue bands, while the second peak is longer-lasting and more luminous in the red and near-infrared (NIR) bands. During the first peak, the spectrum shows a blue continuum with narrow emission lines of H and Fe II. During the second peak, the spectrum becomes cooler, resembling that of a K-type star, and the emission lines are replaced by a forest of narrow lines in absorption. About 5 months later, while the optical light curves are characterized by a fast linear decline, the NIR ones show a moderate rebrightening, observed until the transient disappears in solar conjunction. At these late epochs, the spectrum becomes reminiscent of that of M-type stars, with prominent molecular absorption bands. The late-time properties suggest the formation of some dust in the expanding common envelope or an IR echo from foreground pre-existing dust. We propose that the object is a common-envelope transient, possibly the outcome of a merging event in a massive binary, similar to NGC 4490−2011OT1 .

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 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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.227
Threshold uncertainty score0.654

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 integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.007
GPT teacher head0.201
Teacher spread0.194 · 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.

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

Citations32
Published2019
Admission routes1
Has abstractyes

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