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...
We have determined precise stellar parameters and lithium abundances in a sample of 117 stars with b...
Context.It is known that the surface lithium abundances of field solar-analog G dwarfs show a larg...
Taking into account blending of the lithium 6108 Å line profile by adjacent rare-earth lines togethe...
As a further step in our Lithium project we present results of abundance determination of some eleme...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
International audienceContext. Accurate spectroscopic lithium abundances are essential in addressing...
Context. Accurate spectroscopic lithium abundances are essential in addressing a variety of open que...
We have analyzed the lithium abundance in the atmospheres of 20 stars that are solar analogues based...
We perform non-LTE calculations of lithium in late-type stars for a wide range of stellar parameters...
Lithium abundances determined by spectral synthesis from both the 6708A resonance line and the 6104 ...
The lithium abundances in metal-poor halo stars are of importance for cosmology, galaxy evolution an...
Lithium abundances determined by spectral synthesis from both the 6708 Å resonance line and the 6104...
We study the non-LTE (non local thermodynamic equilibrium) formation of Li I lines in the spectra of...
Context. We report results from lithium abundance determinations using high resolution spectral anal...
We have determined precise stellar parameters and lithium abundances in a sample of 117 stars with b...
Context.It is known that the surface lithium abundances of field solar-analog G dwarfs show a larg...
Taking into account blending of the lithium 6108 Å line profile by adjacent rare-earth lines togethe...
As a further step in our Lithium project we present results of abundance determination of some eleme...
Aims.Lithium abundances for 19 metal-poor stars are determined using high-resolution spectroscopy. T...
International audienceContext. Accurate spectroscopic lithium abundances are essential in addressing...
Context. Accurate spectroscopic lithium abundances are essential in addressing a variety of open que...
We have analyzed the lithium abundance in the atmospheres of 20 stars that are solar analogues based...
We perform non-LTE calculations of lithium in late-type stars for a wide range of stellar parameters...
Lithium abundances determined by spectral synthesis from both the 6708A resonance line and the 6104 ...
The lithium abundances in metal-poor halo stars are of importance for cosmology, galaxy evolution an...
Lithium abundances determined by spectral synthesis from both the 6708 Å resonance line and the 6104...
We study the non-LTE (non local thermodynamic equilibrium) formation of Li I lines in the spectra of...
Context. We report results from lithium abundance determinations using high resolution spectral anal...
We have determined precise stellar parameters and lithium abundances in a sample of 117 stars with b...
Context.It is known that the surface lithium abundances of field solar-analog G dwarfs show a larg...