Magellanic Clouds Cepheids Fourier decomposition Virtual Observatory Resource

Authors

1. Antonello E.

Published by

CDS

Abstract

The radial velocity and light curves of 24 Cepheids in the Magellanic Clouds, with period in the range 30-134d, were Fourier decomposed with the aim of detecting resonance effects between pulsation modes. The Tables contain the list of stars, the details of the analysis and the Fourier parameters.

Keywords

1. magellanic-clouds
2. variable-stars
3. radial-velocity

Bibliographic source Bibcode

1998A&A...333..L35A

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/333/L35

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/333/L35

Document Object Identifer DOI

doi:10.26093/cds/vizier.33339035

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/333/L35
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/333/L35
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/333/L35

IVOA Table Access TAP

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