New SU UMa-Type Dwarf Nova V344 Pav

Details New SU UMa-Type Dwarf Nova V344 Pav New SU UMa-Type Dwarf Nova V344 Pav

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ibvs.5569....1u&link_type=abstract

Information Bulletin on Variable Stars, 5569, 1.

Physics

1

Photometry

Scientific paper

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.

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