International audienceUsing the cosmological constants derived from WMAP, the standard big bang nucleosynthesis (SBBN) predicts the light elements primordial abundances for 4He, 3He, D, 6Li and 7Li. These predictions are in satisfactory agreement with the observations, except for lithium which displays in old warm dwarfs an abundance depleted by a factor of about 3. Depletions of this fragile element may be produced by several physical processes, in different stellar evolutionary phases, they will be briefly reviewed here, none of them seeming yet to reproduce the observed depletion pattern in a fully convincing way
Thirty years after the first observation of the 7Li isotope in the atmosphere of metal-poor halo sta...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
International audienceUsing the cosmological constants derived from WMAP, the standard big bang nucl...
International audienceUsing the cosmological constants derived from WMAP, the standard big bang nucl...
International audienceUsing the cosmological constants derived from WMAP, the standard big bang nucl...
Recent determinations of the abundance of the light-element Li in very metal-poor stars show that it...
Author Institution: Department of Astronomy, University of Illinois, 1002 W. Green St.; Urbana, IL...
Author Institution: Department of Astronomy, University of Illinois, 1002 W. Green St.; Urbana, IL...
Big Bang nucleosynthesis (BBN) theory predicts the abundances of the light elements D, 3He, 4He, and...
Big Bang nucleosynthesis (BBN) theory predicts the abundances of the light elements D, 3He, 4He, and...
The primordial lithium problem is one of the major outstanding issues in the standard model of the B...
We discuss two scenarios for the galactic chemical evolution of lithium. In one, the primordial 7Li ...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
Thirty years after the first observation of the 7Li isotope in the atmosphere of metal-poor halo sta...
Thirty years after the first observation of the 7Li isotope in the atmosphere of metal-poor halo sta...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
International audienceUsing the cosmological constants derived from WMAP, the standard big bang nucl...
International audienceUsing the cosmological constants derived from WMAP, the standard big bang nucl...
International audienceUsing the cosmological constants derived from WMAP, the standard big bang nucl...
Recent determinations of the abundance of the light-element Li in very metal-poor stars show that it...
Author Institution: Department of Astronomy, University of Illinois, 1002 W. Green St.; Urbana, IL...
Author Institution: Department of Astronomy, University of Illinois, 1002 W. Green St.; Urbana, IL...
Big Bang nucleosynthesis (BBN) theory predicts the abundances of the light elements D, 3He, 4He, and...
Big Bang nucleosynthesis (BBN) theory predicts the abundances of the light elements D, 3He, 4He, and...
The primordial lithium problem is one of the major outstanding issues in the standard model of the B...
We discuss two scenarios for the galactic chemical evolution of lithium. In one, the primordial 7Li ...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
Thirty years after the first observation of the 7Li isotope in the atmosphere of metal-poor halo sta...
Thirty years after the first observation of the 7Li isotope in the atmosphere of metal-poor halo sta...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...