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Cited article:

Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations

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Three-dimensional time-dependent convection model for asteroseismology

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Testing the intrinsic scatter of the asteroseismic scaling relations with Kepler red giants

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Coupling between turbulence and solar-like oscillations: A combined Lagrangian PDF/SPH approach

J. Philidet, K. Belkacem and M.-J. Goupil
Astronomy & Astrophysics 656 A95 (2021)
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The ANTARES code: recent developments and applications

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Journal of Physics: Conference Series 1623 (1) 012016 (2020)
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Asteroseismology of 36 Kepler subgiants – I. Oscillation frequencies, linewidths, and amplitudes

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From solar-like to mira stars: a unifying description of stellar pulsators in the presence of stochastic noise

M S Cunha, P P Avelino and W J Chaplin
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Convective excitation and damping of solar-like oscillations

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Monthly Notices of the Royal Astronomical Society 495 (4) 4904 (2020)
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Non-Hessian method for normal coordinate calculations: Application to evaluate vibrational spectra

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The Amplitude of Solar p-mode Oscillations from Three-dimensional Convection Simulations

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The Astrophysical Journal 880 (1) 13 (2019)
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