ABSTRACT
Cataclysmic variables (CVs) are close binary stars in which the most massive component is a white dwarf (WD) and the companion is usually a more normal star—commonly a main sequence star but occasionally a giant
Cataclysmic variables (CVs) are close binary stars in which the most massive component is a white dwarf (WD) and the companion is usually a more normal star—commonly a main sequence star but occasionally a giant