Long-Term Monitoring of the Short Period SU UMa-Type Dwarf Nova, V844 Herculis
Long-Term Monitoring of the Short Period SU UMa-Type Dwarf Nova, V844 Herculis
We report on time-resolved CCD photometry of four outbursts of a short-period SU UMa-type dwarf nova, V844 Herculis. We successfully determined the mean superhump periods to be 0.05584(64) days, and 0.055883(3) for the 2002 May superoutburst, and the 2006 April-May superoutburst, respectively. During the 2002 October observations, we confirmed that …