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Cataclysmic variable stars
URI:
https://gptkb.org/entity/Cataclysmic_variable_stars
GPTKB entity
Statements (49)
Predicate
Object
gptkbp:instanceOf
gptkb:binary_star_system
gptkb:variable_star
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
gptkb:stellar_classification
gptkb: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
gptkb:19th_century
gptkbp:foundIn
gptkb:Milky_Way
gptkbp:hasComponent
gptkb:white_dwarf
donor star
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
gptkb:white_dwarf
intermediate polars
polars
nova-like variable
gptkbp:variant
irregular
periodic
eruptive
gptkbp:whiteDwarfType
degenerate star
gptkbp:bfsParent
gptkb:Magnetic_Braking
gptkbp:bfsLayer
8
https://www.w3.org/2000/01/rdf-schema#label
Cataclysmic variable stars