The 2011 February superoutburst of the dwarf nova SDSS J112003.40+663632.4

摘要

We report unfiltered photometry of SDSS J112003.40+663632.4 during the 2011 February outburst, which revealed the presence of superhumps with peak-to-peak amplitude of up to 0.22 magnitudes, showing this to be an SU UMa type dwarf nova.The outburst amplitude was 5.4 mags above mean quiescence and it lasted at least 12 days.The mean superhump period during the plateau phase was P_(sh)= 0.07057(19)d.