|
gptkbp:instance_of
|
gptkb:star
|
|
gptkbp:associated_with
|
Supernovae
|
|
gptkbp:can_be
|
Transient
|
|
gptkbp:can_detect
|
gptkb:Space_Telescopes
Ground-based Telescopes
|
|
gptkbp:can_lead_to
|
gptkb:Type_Ia_Supernova
|
|
gptkbp:caused_by
|
Accretion of Material
|
|
gptkbp:characterized_by
|
Sudden Increases in Brightness
|
|
gptkbp:conducts_research_on
|
Cosmic Phenomena
Cosmic Evolution
Galactic Dynamics
Astrophysical Simulations
Stellar Remnants
Astrophysical Jets
Astrophysical Observations
Binary Star Evolution
Accretion Processes
Exotic Stars
High-energy Astrophysics
Nova Mechanisms
Stellar Interactions
Stellar Mass Loss
Stellar Population Studies
|
|
gptkbp:discovered_by
|
1930s
|
|
gptkbp:example
|
gptkb:astronomy
|
|
gptkbp:exhibits
|
Outbursts
Periodic Outbursts
|
|
gptkbp:has_type
|
gptkb:Classical_Novae
gptkb:Recurrent_Novae
gptkb:Z_Cam_Stars
gptkb:SU_UMa_Stars
|
|
gptkbp:has_variations
|
Days to Months
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Cataclysmic Variable
|
|
gptkbp:includes
|
gptkb:Nova
Dwarf Novae
|
|
gptkbp:involves
|
gptkb:White_Dwarf
gptkb:Red_Dwarf
|
|
gptkbp:is_a
|
gptkb:star
|
|
gptkbp:is_associated_with
|
X-ray Binaries
|
|
gptkbp:is_characterized_by
|
Rapid Brightness Changes
|
|
gptkbp:is_essential_for
|
gptkb:cosmology
|
|
gptkbp:is_found_in
|
Binary Systems
|
|
gptkbp:is_influenced_by
|
Magnetic Fields
Gravitational Forces
|
|
gptkbp:is_observed_in
|
Various Galaxies
Optical Wavelengths
X-ray Wavelengths
|
|
gptkbp:is_part_of
|
gptkb:galaxy
|
|
gptkbp:is_related_to
|
gptkb:Accretion_Disks
Mass Transfer
Stellar Evolution
|
|
gptkbp:is_similar_to
|
gptkb:Cepheid_Variables
|
|
gptkbp:is_studied_for
|
Understanding Stellar Dynamics
|
|
gptkbp:is_studied_in
|
gptkb:astronomy
|
|
gptkbp:is_used_in
|
Astrophysical Models
|
|
gptkbp:type
|
gptkb:star
|
|
gptkbp:bfsParent
|
gptkb:star
|
|
gptkbp:bfsLayer
|
4
|