1998 Superoutburst of the Large-Amplitude SU UMa-Type Dwarf Nova WX Ceti
1998 Superoutburst of the Large-Amplitude SU UMa-Type Dwarf Nova WX Ceti
Abstract We observed the 1998 November superoutburst of WX Cet, a dwarf nova originally proposed as a WZ Sge-like system. The observation established that WX Cet is an SU UMa-type dwarf nova with a mean superhump period of 0.05949(1)d, which is 2.1% longer than the reported orbital period. The lack …