V810 Cen Geneva photometry

DOI

The light curve of the yellow supergiant V810 Centauri in the Geneva photometric system has been analysed with Date Compensate Fourier Transform and Weighted Wavelet Z-transform. Two periods around 150 and 100 days dominate the frequency spectrum but variable amplitudes and other modes are required to fully reproduce whole data set.

Identifier
DOI http://doi.org/10.26093/cds/vizier.33370779
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/337/779
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/337/779
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/337/779
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/337/779
Provenance
Creator Kienzle F.; Burki G.; Burnet M.; Meynet G.
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy