KnowraCataclysmic variable starLinked fromLinked fromThe 11 pages that link to Cataclysmic variable star, each with the reason it gives.All 11Broader topic 5Related 3Compared with 3White dwarfRelated: Its changing brightness reveals how accretion affects white dwarfs.Accretion diskBroader topic: The transferred matter commonly forms a disk whose changing brightness produces eruptions.Variable starBroader topic: Accretion and eruptions create especially dramatic intrinsic variability.X-ray binaryCompared with: Its accretor is a white dwarf, unlike the neutron stars and black holes considered here.Roche-lobe overflowBroader topic: Many systems feed the white dwarf through sustained Roche-lobe overflow.Roche lobeBroader topic: The donor commonly loses gas after expanding to fill its Roche lobe.Scorpius X-1Compared with: Both systems involve accretion, but Scorpius X-1’s accretor is a neutron star, not a white dwarf.Time-domain astronomyBroader topic: Its recurring eruptions show how monitoring distinguishes repeated activity from one-off transients.Cyclotron radiationRelated: In magnetic systems, cyclotron emission traces hot accretion flows near the white dwarf.Flare starCompared with: Its eruptions commonly involve accretion, unlike flares from a star’s magnetic atmosphere.Common envelopeRelated: Many proposed formation histories require a common envelope to shrink the progenitor orbit.