Statements (43)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:associatedWith |
the_Scorpius_constellation
|
| gptkbp:beam |
is a member of the class of X-ray binaries
|
| gptkbp:collaborations |
studied by multiple international teams
subject of collaborative studies across disciplines |
| gptkbp:companionPlants |
main-sequence star
|
| gptkbp:engagements |
high accretion rate observed
|
| gptkbp:established |
Bruce G. Elmegreen
|
| gptkbp:firstFlight |
identified as an X-ray source
|
| gptkbp:hasResearchFocus |
pivotal in X-ray binaries research
|
| gptkbp:historicalResearch |
continues to be a focus for future research
|
| gptkbp:historicalSignificance |
first X-ray binary discovered
|
| https://www.w3.org/2000/01/rdf-schema#label |
Scorpius X-1
|
| gptkbp:influence |
contributes to understanding of accretion processes
|
| gptkbp:is_monitored_by |
shows rapid variability in X-ray emissions
|
| gptkbp:isInfluencedBy |
frequent X-ray flares observed
|
| gptkbp:issueDate |
surrounds the black hole
|
| gptkbp:length |
approximately 2.7 kiloparsecs
|
| gptkbp:lighting |
approximately 1000 times that of the Sun
exhibits variability in brightness |
| gptkbp:locatedIn |
constellation_Scorpius
|
| gptkbp:model |
used to test theoretical models of black holes
|
| gptkbp:notableFor |
being one of the brightest X-ray sources
|
| gptkbp:notableTracks |
occurs from the companion star
|
| gptkbp:officialResidence |
utilizes advanced observational techniques
collected from various space telescopes |
| gptkbp:orbitalInclination |
approximately 0.787 days
|
| gptkbp:powerOutput |
emits high-energy X-rays
|
| gptkbp:productionCompany |
approximately 0.5 solar masses
|
| gptkbp:releaseYear |
1962
|
| gptkbp:researchAreas |
analyzed for spectral characteristics
|
| gptkbp:researchFocus |
strong X-ray source
|
| gptkbp:researchInterest |
key target for astrophysical research
numerous publications in scientific literature |
| gptkbp:scientificName |
important for studying black hole formation
|
| gptkbp:type |
stellar black hole
O9.5V stellar-mass black hole |
| gptkbp:universe |
demonstrates effects of strong gravity
|
| gptkbp:vision |
provides insights into stellar evolution processes
|
| gptkbp:visitedBy |
gptkb:NASA's_Chandra_X-ray_Observatory
European_Space_Agency's_XMM-Newton |
| gptkbp:weight |
approximately 2.7 solar masses
|