International audienceContext. A discrepancy has emerged between the cosmic lithium abundance inferred by the WMAP satellite measurement coupled with the prediction of the standard big-bang nucleosynthesis theory, and the constant Li abundance measured in metal-poor halo dwarf stars (the so-called Spite plateau). Several models are being proposed to explain this discrepancy, involving either new physics, in situ depletion, or the efficient depletion of Li in the pristine Galaxy by a generation of massive first stars. The realm of possibilities may be narrowed considerably by observing stellar populations in different galaxies, which have experienced different evolutionary histories. Aims: The omega Centauri stellar system is commonly consi...
The ESA Gaia astrometric mission has enabled the remarkable discovery that a large fraction of the s...
The cosmological Li problem is the observed discrepancy between Li abundance (A(Li)) measured in Gal...
The cosmological Li problem is the observed discrepancy between Li abundance (A(Li)) measured in Gal...
International audienceContext. A discrepancy has emerged between the cosmic lithium abundance inferr...
International audienceContext. A discrepancy has emerged between the cosmic lithium abundance inferr...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
Context. A discrepancy has emerged between the cosmic lithium abundance inferred by the WMAP satell...
We present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the stellar s...
We present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the stellar s...
none6siWe present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the st...
We present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the stellar s...
The ESA Gaia astrometric mission has enabled the remarkable discovery that a large fraction of the s...
The cosmological Li problem is the observed discrepancy between Li abundance (A(Li)) measured in Gal...
The cosmological Li problem is the observed discrepancy between Li abundance (A(Li)) measured in Gal...
International audienceContext. A discrepancy has emerged between the cosmic lithium abundance inferr...
International audienceContext. A discrepancy has emerged between the cosmic lithium abundance inferr...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
International audienceomega Centauri is a massive stellar system which is currently going through th...
Context. A discrepancy has emerged between the cosmic lithium abundance inferred by the WMAP satell...
We present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the stellar s...
We present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the stellar s...
none6siWe present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the st...
We present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the stellar s...
The ESA Gaia astrometric mission has enabled the remarkable discovery that a large fraction of the s...
The cosmological Li problem is the observed discrepancy between Li abundance (A(Li)) measured in Gal...
The cosmological Li problem is the observed discrepancy between Li abundance (A(Li)) measured in Gal...