Variable Stars - EG Cnc
Type WZ Sagittae type Click for lightcurve WZ Sagittae type are a subclass of UGSU dwarf novae in which the interval between super- outbursts is unusually long (that is due to a very low mass-transfer rate), measured in decades, while normal outbursts are few and far between. They show re-brightenings. Orbital periods range from 0.05 to 0.08 d. AAVSO Legacy Cataclysmic Variable Programme
Hills Observatory: 1 January 2013 to 6 May 2018
COMETS COMETS
DEEP SKY DEEP SKY