activity
20112022
most citedThree-Dimensional Simulations of Massive Stars: I. Wave Generation and Propagation

103 citations · 636 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2022★ 10 cited

The near-core rotation of HD 112429: a gamma Doradus star with TESS photometry and legacy spectroscopy

T. Van Reeth, P. De Cat, J. Van Beeck +8

The TESS space mission provides us with high-precision photometric observations of bright stars over more than 70% of the entire sky, allowing us to revisit and characterise well-k…

astro-ph.SR2021★ 20 cited

The traditional approximation of rotation for rapidly rotating stars and planets. I. The impact of strong deformation

Hachem Dhouib, Vincent Prat, Timothy Van Reeth +1

The Traditional Approximation of Rotation (TAR) is a treatment of the hydrodynamic equations of rotating and stably stratified fluids in which the action of the Coriolis accelerati…

astro-ph.SR2021★ 6 cited

Anisotropic turbulent transport with horizontal shear in stellar radiative zones

Vincent Prat, Stéphane Mathis

Context. Turbulent transport in stellar radiative zones is a key ingredient of stellar evolution theory, but the anisotropy of the transport due to the stable stratification and th…

astro-ph.SR2020★ 1 cited

Probing the internal magnetism of stars using asymptotic magneto-asteroseismology

Stéphane Mathis, Lisa Bugnet, Vincent Prat +3

Our knowledge of the dynamics of stars has undergone a revolution thanks to the simultaneous large amount of high-quality photometric observations collected by space-based asterose…

astro-ph.SR2020

The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars

L. Bugnet, V. Prat, S. Mathis +5

Stars more massive than M are known to develop a convective core during the main-sequence: the dynamo process triggered by this convection could be the origin of…

astro-ph.SR2020★ 25 cited

Horizontal shear instabilities in rotating stellar radiation zones: II. Effects of the full Coriolis acceleration

Junho Park, Vincent Prat, Stéphane Mathis +1

Stellar interiors are the seat of efficient transport of angular momentum all along their evolution. Understanding the dependence of the turbulent transport triggered by the shear…