Statements (61)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:medical_imaging
gptkb:star |
| gptkbp:analysis |
involves complex modeling techniques
|
| gptkbp:associated_with |
gptkb:supernova_remnants
|
| gptkbp:collaboration |
involving multiple observatories
NASA and ESA missions |
| gptkbp:collaborations |
with universities and research institutions
with international astrophysics teams |
| gptkbp:collection |
from various space telescopes
|
| gptkbp:community |
actively studies its properties
|
| gptkbp:components |
neutron star and companion star
|
| gptkbp:contains |
gptkb:supermassive_black_hole
companion star |
| gptkbp:coordinates |
in the Milky Way galaxy
|
| gptkbp:discovered_by |
gptkb:NASA
C. B. Markwardt |
| gptkbp:discovery_year |
gptkb:1971
|
| gptkbp:distance_from_earth |
approximately 10,000 light years
|
| gptkbp:emissions_standard |
gptkb:X-rays
|
| gptkbp:energy_spectrum |
shows distinct features
|
| gptkbp:file_system |
present around the neutron star
|
| gptkbp:future_prospects |
ongoing studies planned
|
| gptkbp:has_luminosity |
varies with time
between neutron star and companion star |
| gptkbp:has_spectral_type |
varies with observations
|
| gptkbp:historical_significance |
one of the early discovered X-ray binaries
|
| https://www.w3.org/2000/01/rdf-schema#label |
Centaurus X-13
|
| gptkbp:impact |
provides insights into stellar evolution
enhances knowledge of compact objects |
| gptkbp:impact_on_understanding |
of binary star systems
|
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
|
| gptkbp:lighting |
monitored over time
high-energy X-rays shows periodic variations |
| gptkbp:located_in |
gptkb:Centaurus_constellation
|
| gptkbp:migration |
from secondary to primary star
|
| gptkbp:model |
developed to explain its behavior
|
| gptkbp:next_event |
planned with next-generation telescopes
|
| gptkbp:notable_for |
its X-ray emissions
|
| gptkbp:orbital_period |
approximately 5.5 days
|
| gptkbp:power_source |
high during outbursts
|
| gptkbp:primary_star_type |
gptkb:Supernova
|
| gptkbp:provides_information_on |
among global research teams
|
| gptkbp:public_interest |
due to its unique characteristics
|
| gptkbp:publications |
numerous papers published
|
| gptkbp:research |
collected over decades
due to distance and brightness variations documented since its discovery. focused on accretion processes includes X-ray timing and spectroscopy |
| gptkbp:research_importance |
important for studying neutron stars
|
| gptkbp:secondary_star_type |
gptkb:main-sequence_star
|
| gptkbp:sensor |
in 1971
|
| gptkbp:system |
similar to other X-ray binaries
|
| gptkbp:type |
gptkb:medical_imaging
gptkb:supermassive_black_hole |
| gptkbp:variable_star |
yes
|
| gptkbp:x-ray_binaries |
part of the class of X-ray binaries
|
| gptkbp:x-ray_flare |
observed during studies
|
| gptkbp:x-ray_outbursts |
characterized by sudden increases in brightness
|
| gptkbp:x-ray_spectra |
analyzed for understanding composition
|