Add to ORKGWe review general characteristics of massive stars, present the main observable constraints that ste...
Understanding the nature of the first stars is key to understanding the early universe. With new fac...
While the evolution of massive stars in the local Universe is dominated by mass-loss, the evolution ...
Context. Aims.We examine the role of rotation on the evolution and chemical yields of very metal-po...
We review some important observed properties of massive stars. Then we discuss how mass loss and rot...
We discuss the impact of the inclusion of both mass loss and rotation in massive star models at diff...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
Context. Although still beyond our observational abilities, Population III stars are interesting obj...
Grids of models of massive stars ($M \ge$ 20 $M_\odot$) with rotation are computed for metallicitie...
Context. Massive star evolution remains only partly constrained. In particular, the exact role of ro...
The Magellanic Clouds are great laboratories to study the evolution of stars at two metallicities lo...
Mass loss and axial rotation are playing key roles in shaping the evolution of massive stars. They a...
Aims. Many topical astrophysical research areas, such as the properties of planet host stars, the na...
Massive stars played a key role in the early evolution of the Universe. They formed with the first h...
[abridged] Many topical astrophysical research areas, such as the properties of planet host stars, t...
We review general characteristics of massive stars, present the main observable constraints that ste...
Understanding the nature of the first stars is key to understanding the early universe. With new fac...
While the evolution of massive stars in the local Universe is dominated by mass-loss, the evolution ...
Context. Aims.We examine the role of rotation on the evolution and chemical yields of very metal-po...
We review some important observed properties of massive stars. Then we discuss how mass loss and rot...
We discuss the impact of the inclusion of both mass loss and rotation in massive star models at diff...
International audienceContext. Massive star evolution remains only partly constrained. In particular...
Context. Although still beyond our observational abilities, Population III stars are interesting obj...
Grids of models of massive stars ($M \ge$ 20 $M_\odot$) with rotation are computed for metallicitie...
Context. Massive star evolution remains only partly constrained. In particular, the exact role of ro...
The Magellanic Clouds are great laboratories to study the evolution of stars at two metallicities lo...
Mass loss and axial rotation are playing key roles in shaping the evolution of massive stars. They a...
Aims. Many topical astrophysical research areas, such as the properties of planet host stars, the na...
Massive stars played a key role in the early evolution of the Universe. They formed with the first h...
[abridged] Many topical astrophysical research areas, such as the properties of planet host stars, t...
We review general characteristics of massive stars, present the main observable constraints that ste...
Understanding the nature of the first stars is key to understanding the early universe. With new fac...
While the evolution of massive stars in the local Universe is dominated by mass-loss, the evolution ...