Chemical abundances of 257 giant stars

We performed a uniform and detailed abundance analysis of 12 refractory elements for a sample of 257 G- and K-type evolved stars from the CORALIE planet search program. This sample, being homogeneously analyzed, can be used as a comparison sample for other planet-related studies, as well as for different type of studies related to stellar and Galaxy astrophysics. The abundances of the chemical elements were determined using an LTE abundance analysis relative to the Sun, with the spectral synthesis code MOOG and a grid of Kurucz ATLAS9 atmospheres. To separate the Galactic stellar populations both a purely kinematical approach and a chemical method were applied.

Cone search capability for table J/MNRAS/450/1900/stars (Combined table from original tables)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/450/1900
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/450/1900
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/450/1900
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/450/1900
Provenance
Creator Adibekyan V.Zh.; Sousa S.G.; Santos N.C.; Delgado Mena E.,Gonzalez Hernandez J. I.; Israelian G.; Mayor M.; Khachatryan G.,Adibekyan V.; Benamati L.; Alves S.; Lovis C.; Udry S.,Israelian G.; Tsantaki M.; Mortier A.; Sozzetti A.,De Medeiros J.R.
Publisher CDS
Publication Year 2015
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Physics; Solar System Astronomy; Stellar Astronomy