Differential photometry of WX Cet Virtual Observatory Resource

Authors
  1. Sterken C.
  2. Vogt N.
  3. Uemura M.
  4. Tuvikene T.
  5. Published by
    CDS
Abstract

WX Cet is a dwarf nova with rare outbursts of large amplitude. We compile the available data of WX Cet, compare the results with other SU UMa stars, and discuss our findings in the context of current theories of superhumps and superoutbursts to progress with our understanding of SU UMa stars.

Keywords
  1. variable-stars
  2. dwarf-stars
  3. novae
  4. photometry
Bibliographic source Bibcode
2007A&A...463.1053S
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/463/1053
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/463/1053
Document Object Identifer DOI
doi:10.26093/cds/vizier.34631053

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/463/1053
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/463/1053
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/463/1053
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2007-06-17T07:58:51Z
Resource record created
2007-06-17T07:58:51Z
Created
2017-06-02T08:37:23Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr