We present the results of our abundance analysis of Fe, Ni, and O in high signal-to-noise ratio, high-resolution Very Large Telescope UVES and McDonald 2dcoudé spectra of nine dwarfs and three giants in the Hyades open cluster. The difference in Fe abundances derived from F
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
Context. Classical chemical analyses may be affected by systematic errors that would cause observed...
We report a comprehensive light-element (Li, C, N, O, Na, Mg, and Al) abundance analysis of three so...
We present the results of our abundance analysis of Fe, Ni, and O in high signal-to-noise ratio, hig...
We present observations of the 6300 Å [O I] spectral region in two cool Hyades dwarfs, vB 79 and vB ...
Recent LTE analyses (Israelian et al. 1998 and Bosegaard et al. 1999) of the OH bands in the optical...
We present oxygen abundances of dwarfs in the young open cluster IC 4665 deduced from the O I lambda...
We consider potential systematic effects on oxygen abundances derived from the 6300 A (OI) line and ...
Aims. Abundances of 15 chemical elements have been derived for 28 F and 16 A stars members of the Hy...
Received; accepted Aims. Abundances of 15 chemical elements have been derived for 28 F and 16 A star...
Oxygen abundances have been derived from the near-IR, high-excitation O i k7774 triplet in high-reso...
We present oxygen abundances for 72 F and G dwarf stars in the solarneighbourhood. Using the kinemat...
The debate on the oxygen abundances of metal-poor stars has its origin in contradictory results obta...
Oxygen abundances of 67 dwarf stars in the metallicity range -1.6 < [Fe/H] < -0.4 are derived ...
Context. Open clusters are ideal test particles for studying the chemical evolution of the Galactic ...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
Context. Classical chemical analyses may be affected by systematic errors that would cause observed...
We report a comprehensive light-element (Li, C, N, O, Na, Mg, and Al) abundance analysis of three so...
We present the results of our abundance analysis of Fe, Ni, and O in high signal-to-noise ratio, hig...
We present observations of the 6300 Å [O I] spectral region in two cool Hyades dwarfs, vB 79 and vB ...
Recent LTE analyses (Israelian et al. 1998 and Bosegaard et al. 1999) of the OH bands in the optical...
We present oxygen abundances of dwarfs in the young open cluster IC 4665 deduced from the O I lambda...
We consider potential systematic effects on oxygen abundances derived from the 6300 A (OI) line and ...
Aims. Abundances of 15 chemical elements have been derived for 28 F and 16 A stars members of the Hy...
Received; accepted Aims. Abundances of 15 chemical elements have been derived for 28 F and 16 A star...
Oxygen abundances have been derived from the near-IR, high-excitation O i k7774 triplet in high-reso...
We present oxygen abundances for 72 F and G dwarf stars in the solarneighbourhood. Using the kinemat...
The debate on the oxygen abundances of metal-poor stars has its origin in contradictory results obta...
Oxygen abundances of 67 dwarf stars in the metallicity range -1.6 < [Fe/H] < -0.4 are derived ...
Context. Open clusters are ideal test particles for studying the chemical evolution of the Galactic ...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
Context. Classical chemical analyses may be affected by systematic errors that would cause observed...
We report a comprehensive light-element (Li, C, N, O, Na, Mg, and Al) abundance analysis of three so...
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