High-resolution, high signal-to-noise ratio spectra have been obtained for 32 metal-poor stars. The equivalent widths of Li lambda6708 Angstrom were measured and the lithium abundances were derived. The average lithium abundance of 21 stars on the lithium plateau is 2.33+/-0.02 dex. The Lithium plateau exhibits a marginal trend along metallicity, dA(Li)/d[Fe/H] = 0.12+/-0.06, and no clear trend with the effective temperature. The trend indicates that the abundance of lithium plateau may not be primordial and that a part of the lithium was produced in Galactic Chemical Evolution (GCE).Astronomy & AstrophysicsSCI(E)7ARTICLE5453-457
Context. The chemical evolution of lithium in the Milky Way represents a major problem in modern ast...
Using the method of spectral synthesis we derived the abundances of Li in the atmospheres of 100 sta...
The lithium abundance in 62 halo dwarfs is determined from accurate equivalent widths reported in th...
Abstract High-resolution, high signal-to-noise ratio spectra have been obtained for 32 metal-poor st...
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...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
We have determined Li abundances for eleven metal-poor turnoff stars, among which eight have [Fe/H] ...
We have studied 23 very metal-poor field turnoff stars, specifically chosen to enable a precise meas...
The formation and evolution of light elements in the Universe act as important cosmological constrai...
We present a survey of lithium abundances in 185 main- sequence field stars with Teff between 5600 a...
Context. The chemical evolution of lithium in the Milky Way represents a major problem in modern ast...
Using the method of spectral synthesis we derived the abundances of Li in the atmospheres of 100 sta...
The lithium abundance in 62 halo dwarfs is determined from accurate equivalent widths reported in th...
Abstract High-resolution, high signal-to-noise ratio spectra have been obtained for 32 metal-poor st...
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...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
International audienceWe discuss the current status of the sample of Lithium abundances in extremely...
We have determined Li abundances for eleven metal-poor turnoff stars, among which eight have [Fe/H] ...
We have studied 23 very metal-poor field turnoff stars, specifically chosen to enable a precise meas...
The formation and evolution of light elements in the Universe act as important cosmological constrai...
We present a survey of lithium abundances in 185 main- sequence field stars with Teff between 5600 a...
Context. The chemical evolution of lithium in the Milky Way represents a major problem in modern ast...
Using the method of spectral synthesis we derived the abundances of Li in the atmospheres of 100 sta...
The lithium abundance in 62 halo dwarfs is determined from accurate equivalent widths reported in th...