New constraints on stellar models are provided by large surveys of massive stars, interferometric observations and asteroseismology. After a review of the main results so far obtained, we present new results from rotating models and discuss comparisons with observed features. We conclude that rotation is a key feature of massive star physics
Mass loss and axial rotation are playing key roles in shaping the evolution of massive stars. They a...
We investigate the evolution of the surface properties of models for rotating massive stars, i.e., t...
Massive stars play a major role not only in stellar evolution but also galactic evolution theory. Th...
New constraints on stellar models are provided by large surveys of massive stars, interferometric ob...
Context. Massive star evolution remains only partly constrained. In particular, the exact role of ro...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
The Be star phenomenon is related to fast rotation, although the cause of this fast rotation is not ...
After highlighting the principle and power of asteroseismology for stellar physics, we briefly empha...
Some useful developments in the model physics are briefly presented, followed by model results on ch...
After a brief review of the observational evidences indicating how the populations of Be stars, red/...
Context. Rotation plays a key role in the life cycles of stars with masses above ~8 M⊙. Hence, acc...
Some useful developments in the model physics are briefly presented, followed by model results on ch...
We present a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence star...
In addition to being spectacular objects, Very Massive Stars (VMS) are suspected to have a tremendou...
The evolutionary models of massive stars that are widely used in various branches of astronomy are s...
Mass loss and axial rotation are playing key roles in shaping the evolution of massive stars. They a...
We investigate the evolution of the surface properties of models for rotating massive stars, i.e., t...
Massive stars play a major role not only in stellar evolution but also galactic evolution theory. Th...
New constraints on stellar models are provided by large surveys of massive stars, interferometric ob...
Context. Massive star evolution remains only partly constrained. In particular, the exact role of ro...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
The Be star phenomenon is related to fast rotation, although the cause of this fast rotation is not ...
After highlighting the principle and power of asteroseismology for stellar physics, we briefly empha...
Some useful developments in the model physics are briefly presented, followed by model results on ch...
After a brief review of the observational evidences indicating how the populations of Be stars, red/...
Context. Rotation plays a key role in the life cycles of stars with masses above ~8 M⊙. Hence, acc...
Some useful developments in the model physics are briefly presented, followed by model results on ch...
We present a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence star...
In addition to being spectacular objects, Very Massive Stars (VMS) are suspected to have a tremendou...
The evolutionary models of massive stars that are widely used in various branches of astronomy are s...
Mass loss and axial rotation are playing key roles in shaping the evolution of massive stars. They a...
We investigate the evolution of the surface properties of models for rotating massive stars, i.e., t...
Massive stars play a major role not only in stellar evolution but also galactic evolution theory. Th...