Galactic thin disk [Th/Eu] abundance ratios Virtual Observatory Resource

Authors

1. del Peloso E.F.
2. da Silva L.
3. Porto de Mello G.F.

Published by

CDS

Abstract

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.

Keywords

1. late-type-stars
2. chemically-peculiar-stars

Bibliographic source Bibcode

2005A&A...434..275D

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/434/275

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/434/275

Document Object Identifer DOI

doi:10.26093/cds/vizier.34340275

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/434/275
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/434/275
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/434/275

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/434/275/stars?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/434/275/stars?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/434/275/stars?