Walraven photometry of WX Hyi Virtual Observatory Resource

Authors

1. Kuulkers E.
2. Hollander A.
3. Oosterbroeck T.
4. van Paradijs J.

Published by

CDS

Abstract

The SU UMa-type dwarf nova WX Hyi was observed in the 5 passbands VBLUW (544, 430, 384, 362 and 324nm) during 15 nights on the 90cm telescope at ESO (La Silla), between July and November 1988, with an integration time of 16s.

Keywords

1. variable-stars
2. visible-astronomy
3. Wide-band photometry
4. cataclysmic-variable-stars

Bibliographic source Bibcode

1991A&A...242..401K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/242/401

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/242/401

Document Object Identifer DOI

doi:10.26093/cds/vizier.32420401

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/242/401
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/242/401
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/242/401

IVOA Table Access TAP

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