Search Results - "Ong, J. M. Joel"
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Mode Mixing and Rotational Splittings. II. Reconciling Different Approaches to Mode Coupling
Published in The Astrophysical journal (01-04-2023)“…Abstract In the mixed-mode asteroseismology of subgiants and red giants, the coupling between the p- and g- mode cavities must be understood well in order to…”
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Investigating the Metallicity-Mixing-length Relation
Published in The Astrophysical journal (01-05-2018)“…Stellar models typically use the mixing-length approximation as a way to implement convection in a simplified manner. While conventionally the value of the…”
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3
Red Giant Rotational Inversion Kernels Need Nonlinear Surface Corrections
Published in The Astrophysical journal (01-01-2024)“…Abstract Asteroseismology is our only means of measuring the rotations of stars in their interiors, rather than at their surfaces. Some techniques for…”
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Mixed Modes and Asteroseismic Surface Effects. I. Analytic Treatment
Published in The Astrophysical journal (01-10-2021)“…Abstract Normal-mode oscillation frequencies computed from stellar models differ from those that would be measured from stars with identical interior…”
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Evolutionary and Observational Properties of Red Giant Acoustic Glitch Signatures
Published in The Astrophysical journal (01-04-2023)“…Abstract While solar-like oscillations in red giants have been observed at massive scales by the Kepler mission, few features of these oscillation mode…”
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The Gasing Pangkah Collaboration. I. Asteroseismic Identification and Characterization of a Rapidly Rotating Engulfment Candidate
Published in The Astrophysical journal (01-05-2024)“…Abstract We report the discovery and characterization of TIC 350842552 (“Zvrk”), an apparently isolated, rapidly rotating ( P rot ∼ 99 days) red giant observed…”
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Fossil Signatures of Main-sequence Convective Core Overshoot Estimated through Asteroseismic Analyses
Published in The Astrophysical journal (01-04-2024)“…Abstract Some physical processes that occur during a star's main-sequence evolution also affect its post-main-sequence evolution. It is well known that stars…”
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Near-core Acoustic Glitches Are Not Oscillatory: Consequences for Asteroseismic Probes of Convective Boundary Mixing
Published in The Astrophysical journal (01-06-2023)“…Abstract Asteroseismology has been used extensively in recent years to study the interior structure and physical processes of main-sequence stars. We consider…”
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Mode Mixing and Rotational Splittings. I. Near-degeneracy Effects Revisited
Published in The Astrophysical journal (01-11-2022)“…Abstract Rotation is typically assumed to induce strictly symmetric rotational splitting into the rotational multiplets of pure p - and g -modes. However, for…”
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Differential Modeling Systematics across the HR Diagram from Asteroseismic Surface Corrections
Published in The Astrophysical journal (01-01-2021)“…Localized modeling error in the near-surface layers of evolutionary stellar models causes the frequencies of their normal modes of oscillation to differ from…”
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Stellar Models are Reliable at Low Metallicity: An Asteroseismic Age for the Ancient Very Metal-poor Star KIC 8144907
Published in The Astrophysical journal (01-11-2024)“…Abstract Very-metal-poor stars ([Fe/H] < −2) are important laboratories for testing stellar models and reconstructing the formation history of our galaxy…”
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TESS Asteroseismology of β Hydri: A Subgiant with a Born-again Dynamo
Published in The Astrophysical journal (01-10-2024)“…Abstract The solar-type subgiant β Hyi has long been studied as an old analog of the Sun. Although the rotation period has never been measured directly, it was…”
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13
Structural and Evolutionary Diagnostics from Asteroseismic Phase Functions
Published in The Astrophysical journal (01-11-2019)“…In the asymptotic parameterization of mode frequencies, the phase function ϵ( ) completely specifies the detailed structure of the frequency eigenvalues. In…”
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14
Mixed Modes and Asteroseismic Surface Effects. II. Subgiant Systematics
Published in The Astrophysical journal (01-11-2021)“…Abstract Models of solar-like oscillators yield acoustic modes at different frequencies than would be seen in actual stars possessing identical interior…”
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Asteroseismology and Spectropolarimetry of the Exoplanet Host Star λ Serpentis
Published in The Astronomical journal (01-10-2023)“…Abstract The bright star λ Ser hosts a hot Neptune with a minimum mass of 13.6 M ⊕ and a 15.5 day orbit. It also appears to be a solar analog, with a mean…”
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Revisiting the Red Giant Branch Hosts KOI-3886 and ι Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters
Published in The Astronomical journal (01-05-2023)“…Abstract Asteroseismology is playing an increasingly important role in the characterization of red giant host stars and their planetary systems. Here, we…”
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Explaining Deviations from the Scaling Relationship of the Large Frequency Separation
Published in The Astrophysical journal (01-01-2019)“…Asteroseismic large frequency separations possess great diagnostic value. However, their expressions as scaling relations are predicated on homology arguments…”
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Mixed-mode Asteroseismology of Red Giant Stars Through the Luminosity Bump
Published in The Astrophysical journal (01-06-2022)“…Abstract Most current models of low-mass red giant stars do not reproduce the observed position of the red giant branch luminosity bump, a diagnostic of the…”
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Asteroseismic g-mode period spacings in strongly magnetic rotating stars
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT Strong magnetic fields are expected to significantly modify the pulsation frequencies of waves propagating in the cores of red giants or in the…”
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Semianalytic Expressions for the Isolation and Coupling of Mixed Modes
Published in The Astrophysical journal (01-08-2020)“…In the oscillation spectra of giant stars, nonradial modes may be seen to undergo avoided crossings, which produce a characteristic "mode bumping" of the…”
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