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Cited article:

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Transport of angular momentum by stochastically excited waves as an explanation for the outburst of the rapidly rotating Be star HD49330

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Astronomy & Astrophysics 644 A9 (2020)
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A Model of Rotating Convection in Stellar and Planetary Interiors. I. Convective Penetration

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Oscillation frequencies for 35Keplersolar-type planet-hosting stars using Bayesian techniques and machine learning

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SPIN–ORBIT ALIGNMENT OF EXOPLANET SYSTEMS: ENSEMBLE ANALYSIS USING ASTEROSEISMOLOGY

T. L. Campante, M. N. Lund, J. S. Kuszlewicz, G. R. Davies, W. J. Chaplin, S. Albrecht, J. N. Winn, T. R. Bedding, O. Benomar, D. Bossini, R. Handberg, A. R. G. Santos, V. Van Eylen, S. Basu, J. Christensen-Dalsgaard, Y. P. Elsworth, S. Hekker, T. Hirano, D. Huber, C. Karoff, H. Kjeldsen, M. S. Lundkvist, T. S. H. North, V. Silva Aguirre, D. Stello and T. R. White
The Astrophysical Journal 819 (1) 85 (2016)
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Characterizing the propagation of gravity waves in 3D nonlinear simulations of solar-like stars

L. Alvan, A. Strugarek, A. S. Brun, S. Mathis and R. A. Garcia
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Theoretical seismology in 3D: nonlinear simulations of internal gravity waves in solar-like stars

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Angular momentum transport by stochastically excited oscillations in rapidly rotating massive stars

Umin Lee, Coralie Neiner and Stéphane Mathis
Monthly Notices of the Royal Astronomical Society 443 (2) 1515 (2014)
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Angular momentum transport by internal waves in stellar interiors

S. Mathis, G. Alecian, Y. Lebreton, O. Richard and G. Vauclair
EAS Publications Series 63 269 (2013)
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ASTEROSEISMIC DETERMINATION OF OBLIQUITIES OF THE EXOPLANET SYSTEMS KEPLER-50 AND KEPLER-65

W. J. Chaplin, R. Sanchis-Ojeda, T. L. Campante, et al.
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3D simulations of internal gravity waves in solar-like stars

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Proceedings of the International Astronomical Union 9 (S301) 375 (2013)
https://doi.org/10.1017/S1743921313014622