SU UMa Stars

GPTKB entity

Statements (69)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:associated_with gptkb:star
gptkbp:can_cause nova-like outbursts
gptkbp:characterized_by outbursts
gptkbp:discovery first identified in 1970s
gptkbp:exhibits periodic outbursts
gptkbp:has accretion disk
light curve variability
mass transfer process
orbital period variability
red dwarf companion
spectroscopic features
white dwarf component
https://www.w3.org/2000/01/rdf-schema#label SU UMa Stars
gptkbp:includes SU Ursae Majoris
U Geminorum
Z Cha
gptkbp:investigates orbital dynamics
accretion rates
orbital period changes
gptkbp:is_associated_with gptkb:supernova_remnants
stellar flares
gptkbp:is_characterized_by quiescent states
gptkbp:is_essential_for studying binary star interactions
gptkbp:is_examined_in stellar dynamics
stellar population studies
light curve analysis
stellar interaction models
gptkbp:is_found_in constellation Ursa Major
gptkbp:is_known_for brightness variations
high-energy emissions
outburst frequency
outburst mechanisms
rapid brightness changes
gptkbp:is_monitored_by amateur astronomers
spectral changes
light curve patterns
outburst predictions
gptkbp:is_observed_in optical wavelengths
space telescopes
X-ray wavelengths
radio wavelengths
infrared wavelengths
ultraviolet wavelengths
gamma-ray wavelengths
gptkbp:is_part_of gptkb:Milky_Way_galaxy
astrophysical phenomena
stellar populations
stellar evolution theories
cataclysmic variable star class
variable star catalogues
gptkbp:is_related_to stellar evolution
stellar magnetic fields
stellar population synthesis
mass loss in stars
stellar formation processes
accretion phenomena
stellar mass transfer
gptkbp:is_studied_for energy output
stellar interactions
stellar mass distribution
accretion disk physics
gptkbp:is_studied_in astrophysics
stellar astrophysics
gptkbp:is_used_in stellar modeling
gptkbp:scientific_classification gptkb:star
gptkbp:type dwarf nova
gptkbp:bfsParent gptkb:Cataclysmic_Variable
gptkbp:bfsLayer 5