Statements (53)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:associated_with |
gptkb:football_club
|
| gptkbp:contains |
gptkb:physicist
gptkb:star |
| gptkbp:discovered_by |
gptkb:1971
gptkb:NASA |
| gptkbp:distance |
approximately 10,000 light years
|
| gptkbp:emissions_standard |
gptkb:X-rays
|
| gptkbp:exhibition |
X-ray flares
|
| gptkbp:has_luminosity |
10^38 erg/s
|
| gptkbp:has_spectral_type |
O-type star
|
| gptkbp:has_variants |
light curve variability
|
| https://www.w3.org/2000/01/rdf-schema#label |
Centaurus X-10
|
| gptkbp:is_associated_with |
gptkb:supernova_remnants
accretion disks stellar mass black holes |
| gptkbp:is_considered |
stellar dynamics research
|
| gptkbp:is_considered_as |
a prototype of X-ray binaries
|
| gptkbp:is_known_for |
high-energy emissions
its variability in X-ray emissions |
| gptkbp:is_monitored_by |
space telescopes
|
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
gptkb:XMM-Newton optical wavelengths X-ray wavelengths |
| gptkbp:is_part_of |
gptkb:Milky_Way_galaxy
high-energy astrophysics astrophysical phenomena multi-wavelength astronomy X-ray astronomy studies X-ray binary class X-ray binary classification systems X-ray binary evolution studies X-ray binary population studies X-ray binary research |
| gptkbp:is_related_to |
gamma-ray bursts
black hole candidates |
| gptkbp:is_studied_in |
astrophysicists
stellar evolution mass transfer processes its accretion mechanisms |
| gptkbp:is_used_in |
theoretical models of X-ray binaries
|
| gptkbp:lighting |
varies with time
|
| gptkbp:located_in |
gptkb:Centaurus_constellation
Dec -62° 24' 00" RA 12h 10m 32s |
| gptkbp:mass |
greater than 10 solar masses
1.4 solar masses |
| gptkbp:orbital_period |
5.8 days
|
| gptkbp:set_in |
X-ray binary systems category
|
| gptkbp:type |
gptkb:star
X-ray source |
| gptkbp:year |
gptkb:1971
|