Photometric light curves analysis of SU UMa-type dwarf novae: the case of RZ LMi and KV Dra
Abstract
The results of new photometric observations of two SU~UMa type dwarf novae are presented. Superhumps were detected on the light curves of these systems during superoutbursts and their periods and amplitudes determined. The classification of objects as dwarf novae of the ER~UMa subclass (for RZ~LMi) and subclass WZ~Sge (for KV~Dra) has been clarified. Orbital period 0d.0586 for KV Dra was determined.
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