New SU UMa-Type Dwarf Nova V344 Pav
Abstract
We performed time-series observations of a dwarf nova V344 Pav during the outburst on 2004 August. The object showed superhumps, which establish that the object is a new SU UMa-type dwarf nova. We calculate the superhump period to be 0.079607(82) d In conjunction with the reported supercycle of V344 Pav, the relatively long superhump period indicates that it is one of ordinary SU UMa stars.
- Publication:
-
Information Bulletin on Variable Stars
- Pub Date:
- October 2004
- Bibcode:
- 2004IBVS.5569....1U
- Keywords:
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- photometry