Statements (63)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:medical_imaging
gptkb:star |
| gptkbp:analysis |
involves complex algorithms
|
| gptkbp:associated_with |
gptkb:supernova_remnants
|
| gptkbp:binary_period |
approximately 5.5 days
|
| gptkbp:catalogue_name |
1 E 1207.4-5209
|
| gptkbp:collaboration |
international astronomical community
between universities and research centers |
| gptkbp:collaborations |
with other observatories
with astrophysicists worldwide |
| gptkbp:collaborative_projects |
involving multiple institutions
|
| gptkbp:collection |
ongoing from various missions
|
| gptkbp:community |
actively studying its properties
|
| gptkbp:conference |
discussed in astrophysics meetings
|
| gptkbp:contains |
gptkb:supermassive_black_hole
|
| gptkbp:discovered_by |
gptkb:NASA
|
| gptkbp:discovery |
X-ray astronomy
|
| gptkbp:distance_from_earth |
approximately 10,000 light years
|
| gptkbp:educational_value |
used in academic courses
|
| gptkbp:file_system |
present around the neutron star
|
| gptkbp:first_appearance |
gptkb:1971
|
| gptkbp:future_prospects |
ongoing studies in astrophysics
|
| gptkbp:has_implications_for |
for understanding cosmic phenomena
|
| gptkbp:has_luminosity |
varies with time
influences surrounding stars |
| gptkbp:has_spectral_type |
varies with observations
|
| gptkbp:historical_interpretation |
requires interdisciplinary approaches
|
| gptkbp:historical_significance |
first detected X-ray source in Centaurus constellation
|
| https://www.w3.org/2000/01/rdf-schema#label |
Centaurus X-11
|
| gptkbp:impact |
contributes to understanding of neutron stars
|
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
|
| gptkbp:lighting |
variable
monitored for changes exhibits variability high energy X-rays |
| gptkbp:located_in |
gptkb:Centaurus_constellation
|
| gptkbp:merchandise |
other X-ray binaries
|
| gptkbp:migration |
occurs from the companion star
|
| gptkbp:model |
used to explain observations
|
| gptkbp:next_event |
planned with next-gen telescopes
|
| gptkbp:notable_feature |
pulsar activity
|
| gptkbp:power_source |
significant X-ray output
|
| gptkbp:primary_star_type |
gptkb:Supernova
|
| gptkbp:provides_information_on |
NASA databases
between research teams |
| gptkbp:public_interest |
featured in astronomy outreach programs
|
| gptkbp:publications |
featured in scientific journals
numerous papers published influences future research directions |
| gptkbp:research |
evolving with technology
requires advanced telescopes collected in multiple wavelengths extensive observational records includes spectroscopy and photometry |
| gptkbp:research_focus |
black hole formation theories
|
| gptkbp:research_importance |
helps understand binary systems
|
| gptkbp:secondary_star_type |
gptkb:main-sequence_star
|
| gptkbp:significance |
important for studying stellar evolution
|
| gptkbp:type |
gptkb:star
X-ray source |
| gptkbp:x-ray_binaries |
part of a larger class of objects.
|
| gptkbp:x-ray_spectra |
analyzed for composition
|
| gptkbp:year |
gptkb:1971
|