Statements (51)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:star
|
gptkbp:contains |
gptkb:football_club
gptkb:star |
gptkbp:depicted_in |
gptkb:physicist
|
gptkbp:discovered_by |
gptkb:NASA
the 1970s |
gptkbp:distance |
approximately 10,000 light years
approximately 4,000 light years |
gptkbp:emissions_standard |
gptkb:X-rays
|
gptkbp:first_appearance |
gptkb:1994
|
gptkbp:game_components |
normal star
|
gptkbp:has_luminosity |
varies with time
greater than 1000 times that of the Sun |
gptkbp:has_spectral_type |
O-type star
|
gptkbp:has_variants |
in X-ray brightness
|
https://www.w3.org/2000/01/rdf-schema#label |
Centaurus X-44
|
gptkbp:is_a |
gptkb:star
|
gptkbp:is_affected_by |
gptkb:observatory
|
gptkbp:is_associated_with |
gptkb:supernova_remnants
stellar mass black holes |
gptkbp:is_considered |
a candidate for future gravitational wave detection
a strong X-ray source an important object for understanding black holes. |
gptkbp:is_known_for |
high-energy emissions
high mass transfer rates |
gptkbp:is_monitored_by |
various space telescopes
|
gptkbp:is_noted_for |
its variability in X-ray emissions
|
gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
multiple wavelengths |
gptkbp:is_part_of |
gptkb:Milky_Way_galaxy
the study of compact objects X-ray astronomy research X-ray binary classification the Centaurus X-ray binary group |
gptkbp:is_related_to |
other X-ray binaries
|
gptkbp:is_studied_in |
astrophysics
stellar evolution its mass transfer dynamics |
gptkbp:lighting |
hard X-ray spectrum
|
gptkbp:located_in |
gptkb:Centaurus_constellation
declination -41° 00' 00" right ascension 12h 50m 00s |
gptkbp:mass |
greater than 10 solar masses
|
gptkbp:orbital_period |
approximately 5.5 days
|
gptkbp:primary_source |
gptkb:football_club
|
gptkbp:research |
black hole formation
accretion processes |
gptkbp:set_in |
the Centaurus constellation
|
gptkbp:storage |
around the black hole
|
gptkbp:type |
gptkb:star
black hole binary system |