Add to ORKGThe spectra of studied stars were obtained with the ELODIE spectrograph at the 1.93-m telescope of the Observatoire de Haute Provence (France). The determination of Cu and Zn abundances was carried out in LTE assumption by model atmosphere method, for Cu the hyperfine structure was taken into account. Cu and Zn abundance trends for thin and thick disk's stars are presented
Aims. To understand the formation and evolution of the different stellar populations within our Gala...
Context. The formation scenario of the Galactic thick disk is an unresolved problem. Chemical abunda...
Abundances of neutron-capture (n - capture) elements in the stars belonging to thin and thick disks ...
We have determined abundances of copper, zinc, sodium, and aluminum in the atmospheres of 172 F, G, ...
We present new observations of copper and zinc abundances in 90 metal-poor stars, belonging to the m...
2012yCat..80880750M - VizieR On-line Data Catalog: J/AZh/88/750. Originally published in: 2011AZh......
Abstract. We analyse recent high-resolution spectroscopic observations of Cu and Zn for stars of dif...
We present a detailed and uniform study of C, S, Zn and Cu abundances in a large set of planet host ...
We present Cu and Zn abundances for 38 FGK stars, mostly dwarfs, spanning a metallicity range betwee...
Aims. We investigate possible relations between the abundances of zinc and the light elements sodium...
An investigation has been done in order increase the understanding of the origin and chemical evolut...
Based on spectra from F and G dwarf stars, we present elementalabundance trends in the Galactic thin...
Zn abundances, derived from a model atmosphere analysis of the λ6362.35 Å $\ion{Zn}{i}$ line, are pr...
Based on spectra from F and G dwarf stars, we present elemental abundance trends in the Galactic th...
Aims. To understand the formation and evolution of the different stellar populations within our Gala...
Context. The formation scenario of the Galactic thick disk is an unresolved problem. Chemical abunda...
Abundances of neutron-capture (n - capture) elements in the stars belonging to thin and thick disks ...
We have determined abundances of copper, zinc, sodium, and aluminum in the atmospheres of 172 F, G, ...
We present new observations of copper and zinc abundances in 90 metal-poor stars, belonging to the m...
2012yCat..80880750M - VizieR On-line Data Catalog: J/AZh/88/750. Originally published in: 2011AZh......
Abstract. We analyse recent high-resolution spectroscopic observations of Cu and Zn for stars of dif...
We present a detailed and uniform study of C, S, Zn and Cu abundances in a large set of planet host ...
We present Cu and Zn abundances for 38 FGK stars, mostly dwarfs, spanning a metallicity range betwee...
Aims. We investigate possible relations between the abundances of zinc and the light elements sodium...
An investigation has been done in order increase the understanding of the origin and chemical evolut...
Based on spectra from F and G dwarf stars, we present elementalabundance trends in the Galactic thin...
Zn abundances, derived from a model atmosphere analysis of the λ6362.35 Å $\ion{Zn}{i}$ line, are pr...
Based on spectra from F and G dwarf stars, we present elemental abundance trends in the Galactic th...
Aims. To understand the formation and evolution of the different stellar populations within our Gala...
Context. The formation scenario of the Galactic thick disk is an unresolved problem. Chemical abunda...
Abundances of neutron-capture (n - capture) elements in the stars belonging to thin and thick disks ...