activity
20162020
most citedAn algorithm for computing the 2D structure of fast rotating stars

85 citations · 184 across the 6 of their papers we have counts for

collaborators

6 papers

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…

astro-ph.SR2019★ 25 cited

Evolution of rotation in rapidly rotating early-type stars during the main sequence with 2D models

D. Gagnier, M. Rieutord, C. Charbonnel +2

The understanding of the rotational evolution of early-type stars is deeply related to that of anisotropic mass and angular momentum loss. In this paper, we aim to clarify the rota…

astro-ph.SR2019★ 32 cited

Critical angular velocity and anisotropic mass loss of rotating stars with radiation-driven winds

D. Gagnier, M. Rieutord, C. Charbonnel +2

The understanding of the evolution of early-type stars is tightly related to that of the effects of rapid rotation. For massive stars, rapid rotation combines with their strong rad…

astro-ph.SR2018★ 9 cited

The evolved fast rotator Sargas. Stellar parameters and evolutionary status from VLTI/PIONIER and VLT/UVES

Armando Domiciano de Souza, Kévin Bouchaud, Michel Rieutord +2

Gravity darkening (GD) and flattening are important consequences of stellar rotation. The precise characterization of these effects across the HRD is crucial to a deeper understand…

astro-ph.SR2017★ 11 cited

Gravity darkening in late-type stars. The Coriolis effect

Raphaël Raynaud, Michel Rieutord, Ludovic Petitdemange +2

Recent interferometric data have been used to constrain the brightness distribution at the surface of nearby stars, in particular the so-called gravity darkening that makes fast ro…

astro-ph.SR2016★ 85 cited

An algorithm for computing the 2D structure of fast rotating stars

M. Rieutord, F. Espinosa Lara, B. Putigny

Stars may be understood as self-gravitating masses of a compressible fluid whose radiative cooling is compensated by nuclear reactions or gravitational contraction. The understandi…