Statements (69)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:associated_with |
massive star formation regions
|
| gptkbp:collaborations |
collaborative research efforts
|
| gptkbp:contains |
gptkb:Wolf
gptkb:Supernova |
| gptkbp:contains_star |
gptkb:Giant
|
| gptkbp:discovered_by |
gptkb:Bruce_Balick
|
| gptkbp:discovery_year |
gptkb:1966
gptkb:1967 |
| gptkbp:distance_from_earth |
7,000 light years
about 7,000 light years |
| gptkbp:emissions_standard |
gptkb:X-rays
shows emission lines in spectra |
| gptkbp:file_system |
surrounded by an accretion disk
|
| gptkbp:has_astrophysical_models |
used in astrophysical models
|
| gptkbp:has_astrophysical_phenomena |
associated with various astrophysical phenomena
|
| gptkbp:has_astrophysical_research |
focus of astrophysical research
|
| gptkbp:has_black_hole_candidate |
considered a black hole candidate
|
| gptkbp:has_companion |
neutron star companion
|
| gptkbp:has_discovery_impact |
impact on understanding of black holes
|
| gptkbp:has_energy_output |
high energy output
|
| gptkbp:has_future_research |
subject of future research projects
|
| gptkbp:has_historical_significance |
historically significant in astronomy
|
| gptkbp:has_luminosity |
approximately 100,000 times that of the Sun
about 100,000 times that of the Sun |
| gptkbp:has_mass_loss_rate |
high mass loss rate from the Wolf-Rayet star
|
| gptkbp:has_mass_transfer |
mass transfer from the Wolf-Rayet star
|
| gptkbp:has_observational_challenges |
challenges in observation due to distance
|
| gptkbp:has_observational_data |
extensive observational data available
|
| gptkbp:has_periodicity |
exhibits periodic outbursts
|
| gptkbp:has_publications |
numerous scientific publications
|
| gptkbp:has_radio_wavelength_emission |
detected
|
| gptkbp:has_research_focus |
focus of many astrophysical studies
|
| gptkbp:has_spectral_type |
WC5
|
| gptkbp:has_variations |
in X-ray brightness
exhibits variability in X-ray emissions variability on time scales of seconds to hours |
| gptkbp:has_xray_binaries |
one of the first identified X-ray binaries
|
| gptkbp:has_xray_flare |
known for X-ray flares
|
| gptkbp:has_xray_spectra |
X-ray spectra analyzed
|
| https://www.w3.org/2000/01/rdf-schema#label |
Cygnus X-3
|
| gptkbp:is_associated_with |
gamma-ray bursts
|
| gptkbp:is_considered |
a prototype of microquasars
|
| gptkbp:is_known_for |
its strong X-ray emissions
|
| gptkbp:is_located_at |
declination +40° 57' 00''
right ascension 16h 19m 55.7s |
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
gptkb:Hubble_Space_Telescope |
| gptkbp:is_part_of |
gptkb:the_Milky_Way_galaxy
|
| gptkbp:is_studied_in |
astrophysics
|
| gptkbp:lighting |
light curve shows variability
also emits gamma rays one of the brightest X-ray sources |
| gptkbp:located_in |
constellation Cygnus
|
| gptkbp:mass |
approximately 10 solar masses
about 10 solar masses |
| gptkbp:orbital_period |
about 4.8 hours
4.8 hours |
| gptkbp:primary_star_type |
gptkb:Wolf
|
| gptkbp:public_interest |
of interest to the public and media
|
| gptkbp:radio_wavelength_emission |
strong radio source
|
| gptkbp:research |
spectroscopic data collected
|
| gptkbp:research_importance |
important for understanding binary systems
|
| gptkbp:secondary_star_type |
gptkb:Supernova
|
| gptkbp:significance |
important for studying stellar evolution
|
| gptkbp:type |
gptkb:medical_imaging
microquasar |
| gptkbp:bfsParent |
gptkb:Cygnus
|
| gptkbp:bfsLayer |
5
|