MISHENINA, T. V.; GORBANEVA, T. I.; SOUBIRAN, C.; BIENAYME, O.; KOVTYUKH, V. V.; KOROTIN, S. A.

Metadatos

Licencia de uso del documento

MISHENINA, T. V.
Astronomical observatory of Odessa National University [Odessa]

GORBANEVA, T. I.
Astronomical observatory of Odessa National University [Odessa]

SOUBIRAN, C.
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]

Idioma

Article de revue

Este ítem está publicado en

Odessa Astronomical Publications. 2006, vol. 18, p. 78

AstroPrint

Resumen en inglés

We have carried out the detailed analysis of 350 high-resolution spectra of FGK dwarfs and giants. Abundances of Fe, Si, Ca and Ni have been determined under LTE approximation, whereas abundances of Mg have been determined under NLTE approximation. Spatial velocities with an accuracy better than 1 km/s, as well as orbits, have been computed for dwarfs (or all) stars. They have been used to define 2 subsamples kinematically representative of the thin disk and the thick disk in order to highlight their respective properties. A transition occurs at [Fe/H] = -0.3. Stars more metal-rich than this value have a flat distribution with Zmax<1 kpc and σW<20 km/s, and a narrow distribution of [α/Fe]. There exist stars in this metallicity regime which cannot belong to the thin disk because of their excentric orbits, neither to the thick disk because of their low scale height. Several thin disk stars are identified down to [Fe/H] = - 0.80. Their Mg enrichment is lower than thick disk stars with the same metallicity. Both the dwarfs and the giants show a decrease of [α/Fe] with [Fe/H] in the thick disk.< Leer menos

Palabras clave en inglés

Stars: fundamental parameters

stars: abundances

stars: kinematics

stars: atmospheres

Galaxy: stellar content

Galaxy: stellar content.

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804