Walraven photometry of WX Hyi

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.32420401
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/242/401
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/242/401
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/242/401
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/242/401
Provenance
Creator Kuulkers E.; Hollander A.; Oosterbroeck T.; van Paradijs J.
Publisher CDS
Publication Year 2002
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