The 1994 Superoutburst of UZ Boo

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)

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