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Cited article:

Three-dimensional time-dependent convection model for asteroseismology

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Asteroseismic g-mode period spacings in strongly magnetic rotating stars

Nicholas Z Rui, J M Joel Ong and Stéphane Mathis
Monthly Notices of the Royal Astronomical Society 527 (3) 6346 (2023)
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Coupling between turbulence and solar-like oscillations: A combined Lagrangian PDF/SPH approach

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Modelling the asymmetries of the Sun’s radial p-mode line profiles

J. Philidet, K. Belkacem, R. Samadi, C. Barban and H.-G. Ludwig
Astronomy & Astrophysics 635 A81 (2020)
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Asteroseismology of 36 Kepler subgiants – I. Oscillation frequencies, linewidths, and amplitudes

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Monthly Notices of the Royal Astronomical Society 495 (2) 2363 (2020)
https://doi.org/10.1093/mnras/staa1335

A Model of Rotating Convection in Stellar and Planetary Interiors. II. Gravito-inertial Wave Generation

K. C. Augustson, S. Mathis and A. Astoul
The Astrophysical Journal 903 (2) 90 (2020)
https://doi.org/10.3847/1538-4357/abba1c

Two’s a crowd? Characterising the effect of photometric contamination on the extraction of the global asteroseismic parameter νmax in red-giant binaries

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Red giant stars: from mixed modes to angular momentum

K. Belkacem, A.S. Brun, S. Mathis, C. Charbonnel and B. Dubrulle
EAS Publications Series 82 189 (2019)
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