32 citations · 57 across the 2 of their papers we have counts for
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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…
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…
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…
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…
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…