We investigate two topics regarding solar mass FGK-type stars, the lithium-rotation connection (LRC), and the existence of the 'lithium desert'. We determine the minimum critical rotation velocity (v sin i), related with the LRC separating slow from rapid stellar rotators, to be 5 km s-1. This value also splits different stellar properties. For the first time we explore the behaviour of the LRC for some stellar associations with ages between 45 Myr and 120 Myr. This allows us to study the LRC age dependence at the beginning of the general spin-down stage for low-mass stars, which starts at ∼30-40 Myr. We find that each stellar group presents a characteristic minimum lithium depletion connected to a specific high rotation velocity and that t...
Poster contribution to the SEA XV Scientific Meeting. Lithium abundance is an age indicator for G an...
Context. As a fragile element, lithium is a sensitive probe of physical processes occurring in stell...
Aims. We address the existence and origin of the lithium (Li) desert, a region in the Li–Teff plane ...
We investigate two topics regarding solar mass FGK-type stars, the lithium-rotation connection (LRC)...
We investigate two topics regarding solar mass FGK-type stars, the lithium-rotation connection (LRC)...
A connection between lithium depletion and rotation has been reported for a handful of stellar clust...
International audienceContext. The evolution of lithium abundance in cool dwarfs provides a unique p...
Context. The evolution of lithium abundance in cool dwarfs provides a unique probe of nonstandard pr...
International audienceContext. The evolution of lithium abundance over a star's lifetime is indicati...
A connection between lithium depletion and rotation has been reported for a handful of stellar clust...
Poster contribution to the SEA XV Scientific Meeting. Lithium abundance is an age indicator for G an...
Context. As a fragile element, lithium is a sensitive probe of physical processes occurring in stell...
Aims. We address the existence and origin of the lithium (Li) desert, a region in the Li–Teff plane ...
We investigate two topics regarding solar mass FGK-type stars, the lithium-rotation connection (LRC)...
We investigate two topics regarding solar mass FGK-type stars, the lithium-rotation connection (LRC)...
A connection between lithium depletion and rotation has been reported for a handful of stellar clust...
International audienceContext. The evolution of lithium abundance in cool dwarfs provides a unique p...
Context. The evolution of lithium abundance in cool dwarfs provides a unique probe of nonstandard pr...
International audienceContext. The evolution of lithium abundance over a star's lifetime is indicati...
A connection between lithium depletion and rotation has been reported for a handful of stellar clust...
Poster contribution to the SEA XV Scientific Meeting. Lithium abundance is an age indicator for G an...
Context. As a fragile element, lithium is a sensitive probe of physical processes occurring in stell...
Aims. We address the existence and origin of the lithium (Li) desert, a region in the Li–Teff plane ...