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Record W3101220805 · doi:10.25916/sut.26296003.v1

PSR J2234+0611: A new laboratory for stellar evolution

2024· article· en· W3101220805 on OpenAlexafffund
Kevin Stovall, P. C. C. Freire, John Antoniadis, Manjari Bagchi, J. S. Deneva, N. Garver-Daniels, José Martinez, M. A. McLaughlin, Zaven Arzoumanian, Harsha Blumer, Paul R. Brook, H. Thankful Cromartie, Paul B. Demorest, Megan E. DeCesar, Timothy Dolch, Justin A. Ellis, R. D. Ferdman, E. C. Ferrara, Emmanuel Fonseca, Peter A. Gentile, Megan L. Jones, Michael T. Lam, D. R. Lorimer, Ryan S. Lynch, Cherry Ng, David J. Nice, Timothy T. Pennucci, S. M. Ransom, R. Spiewak, I. H. Stairs, Joseph K. Swiggum, Sarah J. Vigeland, Weiwei Zhu

Bibliographic record

VenueRepository of the Academy's Library (Library of the Hungarian Academy of Sciences) · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of TorontoUniversity of British ColumbiaMcGill University
FundersPrecursory Research for Embryonic Science and TechnologyNatural Sciences and Engineering Research Council of CanadaEuropean CommissionInternational Max Planck Research School for Advanced Methods in Process and Systems EngineeringMax-Planck-GesellschaftInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyNational Science FoundationUniversity of Central FloridaNational Aeronautics and Space Administration
KeywordsPhysicsPulsarOrbital inclinationParallaxAstrophysicsOrbit (dynamics)Orbital elementsProper motionOrbital eccentricityWhite dwarfRadial velocityAstrometryMillisecond pulsarCircular orbitOrbital periodAstronomyStarsBinary number

Abstract

fetched live from OpenAlex

We report the timing results for PSR J2234+0611, a 3.6 ms pulsar in a 32 day, eccentric (e = 0.13) orbit with a helium white dwarf. The precise timing and eccentric nature of the orbit allow measurements of an unusual number of parameters: (a) a precise proper motion of 27.10(3) mas yr-1 and a parallax of 1.05(4) mas resulting in a pulsar distance of 0.95(4) kpc; enabling an estimate of the transverse velocity, 123(5) km s-1. Together with previously published spectroscopic measurements of the systemic radial velocity, this allows a 3D determination of the system's velocity; (b) precise measurements of the rate of advance of periastron yields a total system mass of 1.6518 +0.0033 -0.0035 M o; (c) a Shapiro delay measurement, h 3 = 82 ±14 ns, despite the orbital inclination not being near 90°; combined with the measurement of the total mass yields a pulsar mass of and a companion mass of (d) we measure precisely the secular variation of the projected semimajor axis and detect a significant annual orbital parallax; together these allow a determination of the 3D orbital geometry of the system, including an unambiguous orbital inclination (i = 138.7+2.5 -2.2 deg) and a position angle for the line of nodes (ω = 44+5 -4 deg). We discuss the component masses to investigate the hypotheses previously advanced to explain the origin of eccentric MSPs. The unprecedented determination of the 3D position, motion, and orbital orientation of the system, plus the precise pulsar and WD masses and the latter's optical detection make this system a unique test of our understanding of white dwarfs and their atmospheres.

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 score0.389
Threshold uncertainty score0.938

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.001
Science and technology studies0.0010.001
Scholarly communication0.0000.002
Open science0.0020.001
Research integrity0.0000.001
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 head0.015
GPT teacher head0.236
Teacher spread0.221 · 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

Citations12
Published2024
Admission routes2
Has abstractyes

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