Abundances and equivalent widths of 14 Cepheids Virtual Observatory Resource

Authors

1. Kovtyukh V.V.
2. Andrievsky S.M.
3. Belik S.I.
4. Luck R.E.

Published by

CDS

Abstract

We present the results of a detailed multiphase spectroscopic analysis of 14 classical Cepheids with pulsation periods longer than 10 days. For each star, we have derived phased values of effective temperature, surface gravity, microturbulent velocity, and elemental abundances. We show that the elemental abundance results for these Cepheids are consistent for all pulsational phases.

Keywords

1. variable-stars
2. chemical-abundances
3. line-intensities

Bibliographic source Bibcode

2005AJ....129..433K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/129/433

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/129/433

Document Object Identifer DOI

doi:10.26093/cds/vizier.51290433

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/129/433
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/129/433
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/129/433

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/AJ/129/433/table5?
https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/129/433/table5?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/129/433/table5?