Cataclysmic variable stars

GPTKB entity

Statements (49)
Predicate Object
gptkbp:instanceOf variable star
binary star system
gptkbp:accretionDisk present in most systems
gptkbp:accretionFrom donor star to white dwarf
gptkbp:conducts dwarf nova outburst
nova outburst
nova-like outburst
gptkbp:discoveredBy gptkb:John_Russell_Hind
gptkbp:distance hundreds to thousands of light-years
gptkbp:donorStarType stellar classification
red supergiant
gptkbp:emits gptkb:X-rays
ultraviolet light
infrared light
optical light
gptkbp:example gptkb:V1500_Cygni
AM Herculis
SS Cygni
U Geminorum
Z Camelopardalis
gptkbp:firstDescribed 19th century
gptkbp:foundIn gptkb:Milky_Way
gptkbp:hasComponent white dwarf
donor star
https://www.w3.org/2000/01/rdf-schema#label Cataclysmic variable stars
gptkbp:magneticFieldStrength moderate in intermediate polars
strong in polars
weak in non-magnetic systems
gptkbp:massTransfer gptkb:Roche_lobe_overflow
gptkbp:observedBy space telescopes
ground-based telescopes
gptkbp:outburstAmplitude 2 to 6 magnitudes
gptkbp:outburstCause instabilities in accretion disk
gptkbp:outburstDuration days to weeks
gptkbp:periodRange 1.3 hours to 10 hours
gptkbp:powerSource accretion
gptkbp:spectralType varied
gptkbp:studiedIn astrophysics
gptkbp:subclassOf gptkb:nun
white dwarf
intermediate polars
polars
nova-like variable
gptkbp:variant irregular
periodic
eruptive
gptkbp:whiteDwarfType degenerate star
gptkbp:bfsParent gptkb:Magnetic_Braking
gptkbp:bfsLayer 6