Magellanic Clouds Cepheids Fourier decomposition

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.33339035
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/333/L35
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/333/L35
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/333/L35
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/333/L35
Provenance
Creator Antonello E.
Publisher CDS
Publication Year 1998
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; Exoplanet Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy