Statements (62)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:medical_imaging
gptkb:star |
| gptkbp:advances |
aided in its observation.
|
| gptkbp:associated_with |
gamma-ray emissions
|
| gptkbp:availability |
publicly accessible
|
| gptkbp:collaboration |
international astronomical community
various space agencies new discoveries in astrophysics |
| gptkbp:collaborations |
ongoing with various institutions
|
| gptkbp:collapsing_star |
associated with supernova remnants
|
| gptkbp:collection |
utilizes advanced telescopes
|
| gptkbp:community |
actively studying its properties
|
| gptkbp:community_engagement |
increased through outreach programs
|
| gptkbp:contains |
gptkb:supermassive_black_hole
companion star |
| gptkbp:contribution |
enhanced knowledge of X-ray binaries
|
| gptkbp:data_analysis_methods |
evolved over time
|
| gptkbp:discovered_by |
gptkb:NASA
|
| gptkbp:distance_from_earth |
approximately 10,000 light years
|
| gptkbp:emissions_standard |
gptkb:X-rays
|
| gptkbp:energy_spectrum |
characterized by specific features
|
| gptkbp:evolutionary_path |
informs on binary star evolution
|
| gptkbp:file_system |
present
|
| gptkbp:funding |
supported by various grants
|
| gptkbp:future_goals |
to understand accretion processes
|
| gptkbp:future_prospects |
planned for deeper observations
|
| gptkbp:has_implications_for |
for stellar dynamics
|
| gptkbp:has_luminosity |
varies with time
|
| gptkbp:has_spectral_type |
O-type star
|
| gptkbp:historical_significance |
notable in X-ray astronomy
|
| https://www.w3.org/2000/01/rdf-schema#label |
Centaurus X-8
|
| gptkbp:impact |
gptkb:significant
|
| gptkbp:impact_on_understanding |
black hole physics
|
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
|
| gptkbp:lighting |
high energy
key feature in studies shows periodic variations |
| gptkbp:located_in |
gptkb:Centaurus_constellation
|
| gptkbp:mass |
greater than 10 solar masses
estimated through modeling |
| gptkbp:model |
developed to explain behavior
|
| gptkbp:orbital_period |
approximately 5.5 days
|
| gptkbp:part_of |
Galactic Center region
|
| gptkbp:power_source |
high
|
| gptkbp:publications |
numerous studies published
|
| gptkbp:research |
used for analysis
collected in multiple wavelengths present due to distance |
| gptkbp:research_focus |
stellar evolution
|
| gptkbp:research_interest |
high due to unique characteristics
|
| gptkbp:significance |
important for studying black hole formation
|
| gptkbp:spectroscopic_analysis |
conducted to determine properties
|
| gptkbp:system |
other X-ray binaries
|
| gptkbp:travel_time |
considered in observations
|
| gptkbp:type |
gptkb:supermassive_black_hole
gptkb:star |
| gptkbp:variable_star |
yes
|
| gptkbp:x-ray_binaries |
part of the class of X-ray binaries
|
| gptkbp:x-ray_detection |
critical for understanding its nature
|
| gptkbp:x-ray_flare_events |
documented
|
| gptkbp:x-ray_spectra |
analyzed for composition
|
| gptkbp:year |
gptkb:1980s
|