UZ Boo, which had long been suspected to be a WZ Sge-type dwarf nova, finally exhibited a superoutburst for the first time since its 1970 one.
(sorry, under construction ...)
Superhump light curve , which finally revealed the SU UMa-type nature of this dwarf nova. (obtained at Ouda Station, Kyoto University)
HV Vir (1992) paper (PASJ) (PDF)
HV Vir (2002) paper (PASJ) (PDF)
WX Cet: once regarded as a UZ Boo analog
SU UMa-type dwarf novae in general
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