Photometric variability of WR 103 Virtual Observatory Resource

Authors

1. van Genderen A.M.
2. Veijgen S.R.G.
3. van der Hucht K.A.

Published by

CDS

Abstract

We discuss a collection of archival multi-colour photometric data of the variable WC9-type Wolf-Rayet star WR103=HD164270 observed over a time interval of eleven years. The photometric systems used are Walraven VBLUW, Bessel UBV and Stromgren uvby. The purpose is to search for periodicity and to disentangle continuum and line emission variations.

Keywords

1. wolf-rayet-stars
2. ccd-photometry

Bibliographic source Bibcode

2013Ap&SS.345..133V

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/ApSS/345.133

IVOA Identifier IVOID

ivo://CDS.VizieR/J/other/ApSS/345.133

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/ApSS/345.133
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/ApSS/345.133
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/ApSS/345.133

IVOA Table Access TAP

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