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Nuclear Neural Networks: Emulating Late Burning Stages in Core-collapse Supernova Progenitors
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From stellar light to astrophysical insight: automating variable star research with machine learning
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Properties of observable mixed inertial and gravito-inertial modes in γ Doradus stars
Realistic Uncertainties for Fundamental Properties of Asteroseismic Red Giants and the Interplay between Mixing Length, Metallicity, and
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Estimates of (convective core) masses, radii, and relative ages for ∼14 000 Gaia-discovered gravity-mode pulsators monitored by TESS
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Effect of Rotation on Wave Mixing in Intermediate-mass Stars
A. Varghese, R. P. Ratnasingam, R. Vanon, P. V. F. Edelmann, S. Mathis and T. M. Rogers The Astrophysical Journal 970(2) 104 (2024) https://doi.org/10.3847/1538-4357/ad54b5
A calibration point for stellar evolution from massive star asteroseismology
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The ESO UVES/FEROS Large Programs of TESS OB pulsators
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In search of gravity mode signatures in main sequence solar-type stars observed by Kepler
S. N. Breton, H. Dhouib, R. A. García, A. S. Brun, S. Mathis, F. Pérez Hernández, S. Mathur, A. Dyrek, A. R. G. Santos and P. L. Pallé Astronomy & Astrophysics 679 A104 (2023) https://doi.org/10.1051/0004-6361/202346601
Angular momentum transport by magnetic fields in main-sequence stars with Gamma Doradus pulsators
Predictions for Gravity-mode Periods and Surface Abundances in Intermediate-mass Dwarfs from Shear Mixing and Radiative Levitation
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Five young δ Scuti stars in the Pleiades seen with Kepler/K2
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Asteroseismology of a Double-mode High-amplitude δ Scuti Star TIC 448892817
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Internal Rotation and Inclinations of Slowly Pulsating B Stars: Evidence of Interior Angular Momentum Transport