Add to ORKGWhile the evolution of massive stars in the local Universe is dominated by mass-loss, the evolution of massive Population III stars should be dominated by rotation. An important effect of rotation is rotationally-induced chemical mixing that can dramatically change the stellar structure and the nucleosynthesis. This has significant consequences in the predicted explosion types of Population III stars
We list below a few problems whose resolution might bring new lights on the impacts of the first ste...
Observational evidence for rotationally induced mixing in massive stars is summarized. From these ob...
We review general characteristics of massive stars, present the main observable constraints that ste...
Aims. We present a new grid of massive Population III (Pop III) star models including the effects o...
Context. Aims. We present a new grid of massive population III (Pop III) star models including the e...
Context: Population III (Pop III) stars may be fast rotating. An expected consequence of fast rotati...
Mass loss and axial rotation are playing key roles in shaping the evolution of massive stars. They a...
Massive stars played a key role in the early evolution of the Universe. They formed with the first h...
In addition to being spectacular objects, Very Massive Stars (VMS) are suspected to have a tremendou...
Context. Although still beyond our observational abilities, Population III stars are interesting obj...
Massive stars can be considered as cosmic engines. With their high luminosities, strong stellar wind...
After a brief review of the observational evidences indicating how the populations of Be stars, red/...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
The evolutionary models of massive stars that are widely used in various branches of astronomy are s...
We review some important observed properties of massive stars. Then we discuss how mass loss and rot...
We list below a few problems whose resolution might bring new lights on the impacts of the first ste...
Observational evidence for rotationally induced mixing in massive stars is summarized. From these ob...
We review general characteristics of massive stars, present the main observable constraints that ste...
Aims. We present a new grid of massive Population III (Pop III) star models including the effects o...
Context. Aims. We present a new grid of massive population III (Pop III) star models including the e...
Context: Population III (Pop III) stars may be fast rotating. An expected consequence of fast rotati...
Mass loss and axial rotation are playing key roles in shaping the evolution of massive stars. They a...
Massive stars played a key role in the early evolution of the Universe. They formed with the first h...
In addition to being spectacular objects, Very Massive Stars (VMS) are suspected to have a tremendou...
Context. Although still beyond our observational abilities, Population III stars are interesting obj...
Massive stars can be considered as cosmic engines. With their high luminosities, strong stellar wind...
After a brief review of the observational evidences indicating how the populations of Be stars, red/...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
The evolutionary models of massive stars that are widely used in various branches of astronomy are s...
We review some important observed properties of massive stars. Then we discuss how mass loss and rot...
We list below a few problems whose resolution might bring new lights on the impacts of the first ste...
Observational evidence for rotationally induced mixing in massive stars is summarized. From these ob...
We review general characteristics of massive stars, present the main observable constraints that ste...