MN Dra - a SU UMa-type star during its September 2013 superoutburst
Karolina Bakowska, Arkadiusz Olech, Remigiusz Pospieszynski
TL;DR
This paper presents CCD photometry of MN Draconis during its 2013 superoutburst, confirming its classification as an SU UMa-type star through observed superhumps.
Contribution
First detailed CCD photometry confirming superhumps in MN Draconis during a superoutburst, establishing its SU UMa classification.
Findings
Detection of superhumps during the superoutburst
Confirmation of MN Dra as an SU UMa-type star
Observation of normal and superoutbursts in 2013
Abstract
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.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astronomical Observations and Instrumentation · Stellar, planetary, and galactic studies