Galactic thin disk [Th/Eu] abundance ratios

DOI

The objective of this work is the determination of the age of the Galactic disk using Th/Eu nucleocosmochronology. To achieve this objective, it is necessary to obtain the abundances of Th and Eu through spectral synthesis, and to perform the synthesis it is necessary to know the atmospheric parameters and chemical abundances of contaminating elements.

Cone search capability for table J/A+A/434/275/stars (Star positions and magnitudes (from Simbad))

Identifier
DOI http://doi.org/10.26093/cds/vizier.34340275
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/434/275
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/434/275
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/434/275
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/434/275
Provenance
Creator del Peloso E.F.; da Silva L.; Porto de Mello G.F.
Publisher CDS
Publication Year 2005
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; Stellar Astronomy