activity
20002023
most citedGravity darkening in rotating stars

267 citations · 2.4k across the 65 of their papers we have counts for

collaborators

67 papers

astro-ph.SR2023★ 25 cited

The first two-dimensional stellar structure and evolution models of rotating stars

Joey S. G. Mombarg, Michel Rieutord, Francisco Espinosa Lara

Rotation is a key ingredient in the theory of stellar structure and evolution. Until now, stellar evolution codes operate in a 1-D framework for which the validity domain in regard…

astro-ph.SR2023★ 2 cited

Photometric determination of rotation axis inclination, rotation rate, and mass of rapidly rotating intermediate-mass stars

Axel Lazzarotto, Alain Hui-Bon-Hoa, Michel Rieutord

Intermediate-mass stars are often fast rotators, and hence are centrifugally flattened and affected by gravity darkening. To analyse this kind of stars properly, one must turn to 2…

physics.flu-dyn2023★ 9 cited

Internal shear layers in librating spherical shells: the case of attractors

Jiyang He, Benjamin Favier, Michel Rieutord +1

Following our previous work on periodic ray paths (He et al, 2022), we study asymptotically and numerically the structure of internal shear layers for very small Ekman numbers in a…

astro-ph.SR2021★ 27 cited

Predictions for gravity-mode periods and surface abundances in intermediate-mass dwarfs from shear mixing and radiative levitation

Joey S. G. Mombarg, Aaron Dotter, Michel Rieutord +3

The treatment of chemical mixing in the radiative envelopes of intermediate-mass stars has hardly been calibrated so far. Recent asteroseismic studies demonstrated that a constant…

astro-ph.SR2021★ 9 cited

Seismology of Altair with MOST

Cécile Le Dizès, Michel Rieutord, Stéphane Charpinet +2

Altair is the fastest rotating star at less than 10 parsecs from the Sun. Its precise modelling is a landmark for our understanding of stellar evolution with fast rotation, and all…

astro-ph.SR2020★ 22 cited

Oscillations of 2D ESTER models. I. The adiabatic case

D. R. Reese, G. M. Mirouh, F. Espinosa Lara +2

Recent numerical and theoretical considerations have shown that low-degree acoustic modes in rapidly rotating stars follow an asymptotic formula and recent observations of pulsatio…