Nova Tri UBV(RI)c light curves Virtual Observatory Resource

Authors

1. Chochol D.
2. Katysheva N.A.
3. Shugarov S.YU.
4. Volkov I.M.

Published by

CDS

Abstract

We present the UBV(RI)c photometry of the dwarf nova Tri 2008 = OT J023839.1+355648 obtained during its superoutburst started on October 25, 2008. The object can be classified as a WZ Sge-type dwarf nova. The period of early superhumps 0.05307 days was detected in the first 7 days of the superoutburst. The period of ordinary superhumps 0.053663 days, detected in days 8-23 of the superoutburst, is the shortest one among WZ Sge-type objects. After one month, the dwarf nova returned to its pre-outburst state. A sudden increase of activity of the object during its quiescent stage was detected on January 11, 2009.

Keywords

1. novae
2. infrared-photometry
3. visible-astronomy
4. Wide-band photometry

Bibliographic source Bibcode

2009CoSka..39...43C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/CoSka/39.43

IVOA Identifier IVOID

ivo://CDS.VizieR/J/other/CoSka/39.43

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/CoSka/39.43
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/CoSka/39.43
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/CoSka/39.43

IVOA Table Access TAP

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