Add to ORKGAbstract. The effects of rotation on the evolution and properties of low-mass stars are first discussed from the pre-main sequence to the red giant phase. We then briefly indicate how some observational constraints available for these stars can help us progress in our understanding of the dynamical processes at work in stellar interiors. 1
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
The vast majority of stars are formed in clustered environments. However, to date, most rotational e...
Context. Understanding the physical processes that dictate the angular momentum evolution of solar-t...
The effects of rotation on the evolution and properties of low-mass stars are first discussed from t...
We provide a status report on the determination of stellar ages from asteroseismology for stars of v...
The Sun has been known to rotate for more than 4 centuries, and evidence is also available through d...
The evolutionary behaviour of rotating low-mass stars in the mass range 0.2 and 0.9M ⊙ has been inve...
Rotation is ubiquitous at each step of stellar evolution, from star formation to the final stages, a...
We investigated the role of the environment of star-forming regions on the rotational history of low...
3D Stellar Evolution Workshop -- JUL 22-26, 2002 -- UNIV CALIF DAVIS, DEPT APPL SCI, LIVERMORE, CAWO...
There are still significant uncertainties in our understand of convection and rotation in evolved lo...
International audienceContext. Using asteroseismic techniques, it has recently become possible to pr...
Context. Using asteroseismic techniques, it has recently become possible to probe the internal rotat...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
peer reviewedContext. The recent observations of solar-like oscillations in many red giant stars wit...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
The vast majority of stars are formed in clustered environments. However, to date, most rotational e...
Context. Understanding the physical processes that dictate the angular momentum evolution of solar-t...
The effects of rotation on the evolution and properties of low-mass stars are first discussed from t...
We provide a status report on the determination of stellar ages from asteroseismology for stars of v...
The Sun has been known to rotate for more than 4 centuries, and evidence is also available through d...
The evolutionary behaviour of rotating low-mass stars in the mass range 0.2 and 0.9M ⊙ has been inve...
Rotation is ubiquitous at each step of stellar evolution, from star formation to the final stages, a...
We investigated the role of the environment of star-forming regions on the rotational history of low...
3D Stellar Evolution Workshop -- JUL 22-26, 2002 -- UNIV CALIF DAVIS, DEPT APPL SCI, LIVERMORE, CAWO...
There are still significant uncertainties in our understand of convection and rotation in evolved lo...
International audienceContext. Using asteroseismic techniques, it has recently become possible to pr...
Context. Using asteroseismic techniques, it has recently become possible to probe the internal rotat...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
peer reviewedContext. The recent observations of solar-like oscillations in many red giant stars wit...
This thesis presents analyses aimed at understanding the rotational properties of stars at the botto...
The vast majority of stars are formed in clustered environments. However, to date, most rotational e...
Context. Understanding the physical processes that dictate the angular momentum evolution of solar-t...