activity
20232026
most citedAsteroseismic g-mode period spacings in strongly magnetic rotating stars

26 citations · 65 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Extending asteroseismic magnetometry across the diverse landscape of magnetic structures

Nicholas Z. Rui, J. M. Joel Ong, Armand Leclerc +5

Magnetic fields have now been asteroseismically measured in the cores of many red giants. However, most interpretations of these measurements assume that the magnetic field is far…

astro-ph.SR2026

Asteroseismic imprints of strong non-axisymmetric fields in the cores of red giants

Nicholas Z. Rui, J. M. Joel Ong, Armand Leclerc +5

To date, magnetic fields have been asteroseismically measured in nearly one hundred red giant cores. However, most analyses assume weak magnetic fields and slow rotation so that pe…

astro-ph.EP2025

Unified Kraft Break at ~6500 K: A Newly Identified Single-Star Obliquity Transition Matches the Classical Rotation Break

Xian-Yu Wang, Songhu Wang, J. M. Joel Ong

The stellar obliquity transition, defined by a cut separating aligned from misaligned hot Jupiter systems, has long been assumed to coincide with the rotatio…

astro-ph.SR2024★ 8 cited

TESS asteroseismology of Hydri: a subgiant with a born-again dynamo

Travis S. Metcalfe, Jennifer L. van Saders, Daniel Huber +12

The solar-type subgiant Hyi has long been studied as an old analog of the Sun. Although the rotation period has never been measured directly, it was estimated to be near 27 day…

astro-ph.SR2024

Stellar Models are Reliable at Low Metallicity: An Asteroseismic Age for the Ancient Very Metal-Poor Star KIC 8144907

Daniel Huber, Ditte Slumstrup, Marc Hon +15

Very metal-poor stars ([Fe/H]<-2) are important laboratories for testing stellar models and reconstructing the formation history of our galaxy. Asteroseismology is a powerful tool…

astro-ph.IM2024★ 3 cited

Reggae: A Parametric Tuner for PBJam, and a Visualization Tool for Red Giant Oscillation Spectra

J. M. Joel Ong, Martin B. Nielsen, Emily J. Hatt +1

The upcoming second release of PBJam -- a software instrument for fitting normal modes ("peakbagging") -- supplements the simple power-spectrum model used in the first version to a…

astro-ph.SR2024★ 12 cited

The K2 Asteroseismic KEYSTONE sample of Dwarf and Subgiant Solar-Like Oscillators. I: Data and Asteroseismic parameters

Mikkel N. Lund, Sarbani Basu, Allyson Bieryla +19

The KEYSTONE project aims to enhance our understanding of solar-like oscillators by delivering a catalogue of global asteroseismic parameters ( and ) for 173 s…

astro-ph.SR2024★ 16 cited

Rotation at the Fully Convective Boundary: Insights from Wide WD + MS Binary Systems

Federica Chiti, Jennifer L. van Saders, Tyler M. Heintz +5

Gyrochronology, a valuable tool for determining ages of low-mass stars where other techniques fail, relies on accurate calibration. We present a sample of 185 wide ( au) wh…

astro-ph.SR2024

The Gasing Pangkah Collaboration: I. Asteroseismic Identification and Characterisation of a Rapidly-Rotating Engulfment Candidate

J. M. Joel Ong, Marc Teng Yen Hon, Melinda Soares-Furtado +19

We report the discovery and characterisation of TIC 350842552 ("Zvrk"), an apparently isolated, rapidly-rotating () red giant observed by TESS in…

astro-ph.SR2023

Red Giant Rotational Inversion Kernels Need Nonlinear Surface Corrections

J. M. Joel Ong

Asteroseismology is our only means of measuring stellar rotation in their interiors, rather than at their surfaces. Some techniques for measurements of this kind -- "rotational inv…

astro-ph.SR2023★ 26 cited

Asteroseismic g-mode period spacings in strongly magnetic rotating stars

Nicholas Z. Rui, J. M. Joel Ong, Stéphane Mathis

Strong magnetic fields are expected to significantly modify the pulsation frequencies of waves propagating in the cores of red giants or in the radiative envelopes of intermediate-…