Karolina Bakowska, Arkadiusz Olech, Remigiusz Pospieszynski
Published 2016-01-11Version 1
We report CCD photometry of the cataclysmic variable star MN Draconis. During the season of August-September 2013, one normal outburst and one superoutburst were detected. In the light curves of MN Dra clear superhumps were present during September 2013 superoutburst. That fact confirms that the star is a member of SU UMa class.
Comments: 3 pages, 2 figures, to be published in the Proceedings of the XXXVII Meeting of the Polish Astronomical Society
Superoutbursts and Positive Superhumps are Detected During the Standstill in AT Cnc
Superhumps and their Evolution during Superoutbursts
Investigation of superhumps in SU UMa-type dwarf novae based on the observations of TESS
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