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.
  5. 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?

History

2006-01-28T11:42:46Z
Resource record created
2006-01-28T11:42:46Z
Created
2017-12-12T14:45:25Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr