Statements (60)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:star
|
gptkbp:bfsLayer |
2
|
gptkbp:bfsParent |
gptkb:physicist
|
gptkbp:can_be |
mass transfer
orbital periods different spectral types accretion rates different energy outputs different mass ratios different orbital configurations |
gptkbp:can_create |
stellar evolution
|
gptkbp:contains |
gptkb:football_club
gptkb:physicist normal star |
gptkbp:emissions_standard |
gptkb:X-rays
|
gptkbp:exhibits |
X-ray flares
X-ray bursts X-ray variability outflow jets periodic outbursts quiescent states thermal instability |
gptkbp:has_style |
high-mass X-ray binary
low-mass X-ray binary |
https://www.w3.org/2000/01/rdf-schema#label |
X-ray Binary
|
gptkbp:is_analyzed_in |
gptkb:nebula
|
gptkbp:is_associated_with |
gptkb:nebula
accretion disk gamma-ray bursts stellar winds |
gptkbp:is_characterized_by |
high luminosity
|
gptkbp:is_essential_for |
understanding the universe
understanding cosmic rays studying black hole formation |
gptkbp:is_found_in |
binary star systems
galaxies star-forming regions star clusters |
gptkbp:is_involved_in |
stellar interactions
nuclear fusion processes gravitational wave events |
gptkbp:is_observed_in |
various wavelengths
|
gptkbp:is_part_of |
gptkb:active_galactic_nuclei
gptkb:the_Milky_Way X-ray astronomy |
gptkbp:is_related_to |
gptkb:supernova_remnants
stellar dynamics stellar collisions massive star evolution |
gptkbp:is_studied_in |
gptkb:musician
astrophysics observational astronomy cosmic evolution stellar mass evolution of stars |
gptkbp:recognizes |
radio telescopes
X-ray telescopes |
gptkbp:scientific_classification |
gptkb:X-ray_pulsar
gptkb:star X-ray transient |