|
gptkbp:instance_of
|
gptkb:medical_imaging
gptkb:star
|
|
gptkbp:associated_with
|
gptkb:supernova_remnants
|
|
gptkbp:conducts_research_on
|
in astrophysics
|
|
gptkbp:contains
|
gptkb:supermassive_black_hole
|
|
gptkbp:contains_star
|
gptkb:Giant
|
|
gptkbp:discovered_by
|
gptkb:NASA
|
|
gptkbp:distance_from_earth
|
approximately 10,000 light years
|
|
gptkbp:emissions_standard
|
gptkb:X-rays
|
|
gptkbp:file_system
|
yes
|
|
gptkbp:first_appearance
|
in the 1970s
|
|
gptkbp:has_luminosity
|
varies significantly
|
|
gptkbp:has_spectral_type
|
O-type star
|
|
gptkbp:has_variations
|
high-energy emissions
|
|
gptkbp:has_xray_flare
|
yes
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Centaurus X-34
|
|
gptkbp:is_associated_with
|
gptkb:supernova_remnants
gamma-ray emissions
|
|
gptkbp:is_considered
|
a significant source of X-rays.
a key object in X-ray astronomy
a strong X-ray source
|
|
gptkbp:is_essential_for
|
understanding black hole formation
|
|
gptkbp:is_known_for
|
its high-energy emissions
|
|
gptkbp:is_located_near
|
gptkb:Centaurus_A
|
|
gptkbp:is_monitored_by
|
various observatories
X-ray bursts
|
|
gptkbp:is_noted_for
|
its variability
|
|
gptkbp:is_observed_in
|
gptkb:Chandra_X-ray_Observatory
space telescopes
multiple wavelengths
|
|
gptkbp:is_part_of
|
gptkb:the_Milky_Way_galaxy
the study of compact objects
the Centaurus constellation
X-ray binary classification
X-ray binary systems
|
|
gptkbp:is_related_to
|
stellar mass black holes
|
|
gptkbp:is_studied_for
|
stellar evolution
accretion processes
its accretion dynamics
|
|
gptkbp:is_used_in
|
stellar population studies
|
|
gptkbp:is_visible_from
|
gptkb:Earth
|
|
gptkbp:lighting
|
varies with time
|
|
gptkbp:located_in
|
gptkb:Centaurus_constellation
|
|
gptkbp:mass
|
greater than 10 solar masses
|
|
gptkbp:orbital_period
|
about 5.5 days
|
|
gptkbp:part_of
|
Galactic X-ray binary population
|
|
gptkbp:redshift
|
measurable
|
|
gptkbp:type
|
gptkb:supermassive_black_hole
gptkb:star
|