A3526

E610636

A3526 is a massive galaxy cluster in the constellation Centaurus, notable as one of the nearest and most studied rich clusters of galaxies.

All labels observed (1)

Label Occurrences
A3526 canonical 2

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf Abell galaxy cluster ⓘ
galaxy cluster ⓘ
rich galaxy cluster ⓘ
alsoKnownAs Abell 3526 ⓘ
Centaurus Cluster ⓘ
angularSize large apparent size on the sky due to proximity ⓘ
baryonContent significant fraction in hot intracluster gas ⓘ
catalog Abell catalog of rich clusters of galaxies ⓘ
centralGalaxy NGC 4696 ⓘ
centralRegionDominatedBy giant elliptical galaxy NGC 4696 ⓘ
linked to: NGC 4696
clusterType X-ray bright cluster ⓘ
massive cluster ⓘ
nearby cluster ⓘ
constellation Centaurus ⓘ
contains intracluster medium emitting X-rays ⓘ
large population of elliptical galaxies ⓘ
large population of lenticular galaxies ⓘ
discoveredBy George O. Abell (as part of the Abell catalog) ⓘ
distanceFromEarth approximately 160 million light-years ⓘ
approximately 50 Mpc ⓘ
dynamicalState not fully relaxed, shows subcluster mergers ⓘ
environment dense cluster environment ⓘ
galaxyPopulation dominance of early-type galaxies ⓘ
hasCoolingCore yes (cool-core cluster characteristics) ⓘ
hasGravitationalLensing weak lensing signatures detected ⓘ
hasSubstructure complex subclustering in galaxy distribution ⓘ
multiple galaxy subgroups ⓘ
intraclusterMediumTemperature several keV ⓘ
locatedIn southern celestial hemisphere ⓘ
mass on the order of 10^14–10^15 solar masses ⓘ
memberOf Shapley Supercluster region ⓘ
morphologicalType Bautz–Morgan type I–II (often classified as I) cluster ⓘ
notableFor being one of the most studied galaxy clusters ⓘ
being one of the nearest rich clusters of galaxies ⓘ
observedIn X-ray wavelengths ⓘ
optical wavelengths ⓘ
radio wavelengths ⓘ
redshift 0.0104 ⓘ
richnessClass rich cluster ⓘ
usedAs benchmark system for nearby cluster studies ⓘ
usedFor calibration of scaling relations for nearby clusters ⓘ
studies of cluster dynamics ⓘ
studies of galaxy evolution in clusters ⓘ
studies of intracluster medium physics ⓘ
velocityDispersion on the order of 800–1000 km/s ⓘ
xRayEmission peaked toward cluster center ⓘ
xRayLuminosity high ⓘ

How these facts were elicited

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.