V810 Cen Geneva photometry Virtual Observatory Resource

Authors

1. Kienzle F.
2. Burki G.
3. Burnet M.
4. Meynet G.

Published by

CDS

Abstract

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.

Keywords

1. supergiant-stars
2. visible-astronomy
3. narrow-band-photometry

Bibliographic source Bibcode

1998A&A...337..779K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/337/779

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/337/779

Document Object Identifer DOI

doi:10.26093/cds/vizier.33370779

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/337/779
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/337/779
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/337/779

IVOA Table Access TAP

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