Taking into account blending of the lithium 6108 Å line profile by adjacent rare-earth lines together with their spotted surface structure does not appreciably affect lithium abundance estimates for the atmospheres of HD 83368 and HD 60435 but provides a better fit of the observed and stimulated line profiles. Our computed non-LTE corrections reduce the lithium abundance estimates by 0.1-0.2 dex for both stars. Given the uncertainties in the lithium abundances, it is not possible to be certain whether the lithium abundances in map stars, or at least in their spots, exceed the cosmic (primordial) value. © 2002 MAIK "Nauka/Interperiodica"
Context. We report results from lithium abundance determinations using high resolution spectral anal...
The lithium abundances in metal-poor halo stars are of importance for cosmology, galaxy evolution a...
Context. Un-evolved, very metal-poor stars are the most important tracers of the cosmic abundance of...
Taking into account blending of the lithium 6108 Å line profile by adjacent rare-earth lines togethe...
We perform non-LTE calculations of lithium in late-type stars for a wide range of stellar parameters...
We have analyzed the lithium abundance in the atmospheres of 20 stars that are solar analogues based...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
Lithium abundances determined by spectral synthesis from both the 6708A resonance line and the 6104 ...
As a further step in our Lithium project we present results of abundance determination of some eleme...
International audienceContext. Accurate spectroscopic lithium abundances are essential in addressing...
We study the non-LTE (non local thermodynamic equilibrium) formation of Li I lines in the spectra of...
The lithium abundances in metal-poor halo stars are of importance for cosmology, galaxy evolution an...
As a further step in our Lithium project we present results of abundance determination of some elem...
Context. Accurate spectroscopic lithium abundances are essential in addressing a variety of open que...
Lithium abundances determined by spectral synthesis from both the 6708 Å resonance line and the 6104...
Context. We report results from lithium abundance determinations using high resolution spectral anal...
The lithium abundances in metal-poor halo stars are of importance for cosmology, galaxy evolution a...
Context. Un-evolved, very metal-poor stars are the most important tracers of the cosmic abundance of...
Taking into account blending of the lithium 6108 Å line profile by adjacent rare-earth lines togethe...
We perform non-LTE calculations of lithium in late-type stars for a wide range of stellar parameters...
We have analyzed the lithium abundance in the atmospheres of 20 stars that are solar analogues based...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
Lithium abundances determined by spectral synthesis from both the 6708A resonance line and the 6104 ...
As a further step in our Lithium project we present results of abundance determination of some eleme...
International audienceContext. Accurate spectroscopic lithium abundances are essential in addressing...
We study the non-LTE (non local thermodynamic equilibrium) formation of Li I lines in the spectra of...
The lithium abundances in metal-poor halo stars are of importance for cosmology, galaxy evolution an...
As a further step in our Lithium project we present results of abundance determination of some elem...
Context. Accurate spectroscopic lithium abundances are essential in addressing a variety of open que...
Lithium abundances determined by spectral synthesis from both the 6708 Å resonance line and the 6104...
Context. We report results from lithium abundance determinations using high resolution spectral anal...
The lithium abundances in metal-poor halo stars are of importance for cosmology, galaxy evolution a...
Context. Un-evolved, very metal-poor stars are the most important tracers of the cosmic abundance of...