Photometric Study of Selected SU UMa-Type Dwarf Novae
Year: 2010

In this work we present time-resolved photometry of a few poorly-studied dwarf novae during recent superoutbursts. Observations were made using 60-cm telescope of Sternberg Astronomical Institute in Crimea in October-November 2008 and May-June 2009. Superhumps were detected in the light curves of all novae. The amplitudes and periods of detected light variations were calculated. Superhumps evolution was also followed up for all systems