First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented. Oxygen abundances for 63nearby F and G dwarf stars, based on very high resolution spectra (R∼215 000) and high signal-to-noise (S/N>400) of the faint forbidden oxygen line at 6300Å, have been determined. Our findings can be summarized as follows: 1) at [Fe/H] 0 without showing the leveling out that previously has been seen
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
We present oxygen abundances for 72 F and G dwarf stars in the solar neighbourhood. Using the kinem...
We present oxygen abundances for 72 F and G dwarf stars in the solar neighbourhood. Using the kinem...
We present oxygen abundances for 72 F and G dwarf stars in the solarneighbourhood. Using the kinemat...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
International audienceWe derived oxygen abundances for 42 K giants in four fields towards the Galact...
The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby ($d$5500 K ...
The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby (d-0.3, we ...
The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby ($d$5500 K ...
Aims.We spectroscopically characterize the Galactic Bulge to infer its star formation timescale, com...
Aims.We spectroscopically characterize the Galactic Bulge to infer its star formation timescale, com...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
We present oxygen abundances for 72 F and G dwarf stars in the solar neighbourhood. Using the kinem...
We present oxygen abundances for 72 F and G dwarf stars in the solar neighbourhood. Using the kinem...
We present oxygen abundances for 72 F and G dwarf stars in the solarneighbourhood. Using the kinemat...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
Aims. We present a detailed and uniform study of oxygen abundance from two different oxygen lines at...
International audienceWe derived oxygen abundances for 42 K giants in four fields towards the Galact...
The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby ($d$5500 K ...
The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby (d-0.3, we ...
The abundances of iron and oxygen are homogeneously determined in a sample of 523 nearby ($d$5500 K ...
Aims.We spectroscopically characterize the Galactic Bulge to infer its star formation timescale, com...
Aims.We spectroscopically characterize the Galactic Bulge to infer its star formation timescale, com...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...
International audienceAims.We spectroscopically characterize the Galactic Bulge to infer its star fo...