Properties (58)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
black hole
|
| gptkbp:analyzes |
requires advanced data analysis techniques
|
| gptkbp:associatedWith |
theoretical physics
|
| gptkbp:beam |
one of the first identified
|
| gptkbp:collaborations |
international research collaboration
involves multiple institutions |
| gptkbp:companionPlants |
HDE 226868
|
| gptkbp:culturalImpact |
featured in media and literature
|
| gptkbp:educational_programs |
used in educational materials
|
| gptkbp:engagements |
high accretion rate
|
| gptkbp:established |
gptkb:Tom_Bolton
|
| gptkbp:events |
theoretical presence
|
| gptkbp:fanEvents |
not directly related to particle physics
|
| gptkbp:financialPerformance |
discussed in many conferences
|
| gptkbp:firstAppearance |
supports existence of black holes
|
| gptkbp:firstSeason |
to be widely accepted
|
| gptkbp:historicalResearch |
ongoing studies planned
|
| https://www.w3.org/2000/01/rdf-schema#label |
Cygnus X-1
|
| gptkbp:influence |
significant influence on modern astronomy
|
| gptkbp:influencedBy |
general relativity
|
| gptkbp:issueDate |
present
|
| gptkbp:length |
about 6,070 light years
|
| gptkbp:lighting |
about 1.2 million times that of the Sun
variable light curve observed |
| gptkbp:locatedIn |
constellation_Cygnus
|
| gptkbp:model |
used in black hole models
|
| gptkbp:namedAfter |
the_constellation_Cygnus
|
| gptkbp:notableFeature |
studied for black hole formation
|
| gptkbp:notableTracks |
occurs from companion star
|
| gptkbp:officialResidence |
X-ray astronomy
difficult to observe directly collected over decades |
| gptkbp:orbitalInclination |
5.6 days
|
| gptkbp:partOf |
the Milky Way galaxy
|
| gptkbp:powerOutput |
extremely high energy output
|
| gptkbp:publicAccess |
popular in science communication
|
| gptkbp:publications |
widely cited in scientific literature
|
| gptkbp:relatedPatent |
other black holes
|
| gptkbp:releaseYear |
1964
|
| gptkbp:researchAreas |
hard X-ray spectra
|
| gptkbp:researchField |
astrophysics
|
| gptkbp:researchFocus |
strong
|
| gptkbp:researchInterest |
numerous publications exist
|
| gptkbp:scientificName |
important to the scientific community
key to understanding black holes |
| gptkbp:serves |
from companion star
|
| gptkbp:significance |
important for black hole research
|
| gptkbp:stations |
detected
|
| gptkbp:theory |
implications for physics theories
used in various theoretical frameworks |
| gptkbp:type |
X-ray binary system
stellar black hole O9.7 Iab |
| gptkbp:universe |
not detected yet
|
| gptkbp:vision |
related to massive stars
|
| gptkbp:visitedBy |
gptkb:Chandra_X-ray_Observatory
gptkb:Hubble_Space_Telescope |
| gptkbp:weight |
approximately 14.8 solar masses
|