Abell 3526

E481659

Abell 3526, also known as the Centaurus Cluster, is a massive nearby galaxy cluster notable for its rich galaxy population and strong X-ray emission.

All labels observed (1)

Label Occurrences
Abell 3526 canonical 7

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf Abell galaxy cluster
galaxy cluster
alsoKnownAs Centaurus Cluster
BautzMorganType I
catalogCode A3526
centralGalaxyType giant elliptical galaxy
containsGalaxy NGC 4696
NGC 4696A
linked to: NGC 4696

NGC 4696B
NGC 4706
NGC 4709
discoveredBy George O. Abell
distanceFromEarth approximately 170 million light-years
approximately 52 megaparsecs
environment dense cluster environment
hasBrightestClusterGalaxy NGC 4696
hasCoolingFlow yes
hasDarkMatter yes
hasIntraclusterMedium hot gas
hasMemberCount several hundred galaxies
hasRadioSource PKS 1246-410
linked to: NGC 4696
hasSubcluster Cen 30
Cen 45
hasVelocityDispersion about 800–900 km/s
hasXRayEmission strong
isBrightIn X-ray
optical
isDynamicallyComplex yes
isGravitationallyBoundSystem yes
isNearbyCluster yes
locatedInConstellation Centaurus
mass on the order of 10^14–10^15 solar masses
observedBy Chandra X-ray Observatory
Einstein Observatory
ROSAT
XMM-Newton
linked to: XMM-Newton mission
partOf Abell catalogue of rich clusters of galaxies
redshift 0.0104
richnessClass 1
showsMergerActivity yes
temperatureOfIntraclusterMedium about 3–4 keV
usedForStudyOf cluster mergers
cooling flows
galaxy evolution in clusters
intracluster medium
XRayLuminosity high

How these facts were elicited

Referenced by (7)

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

Centaurus Cluster alsoKnownAs Abell 3526
Hydra–Centaurus contains Abell 3526
NGC 4709 isPartOf Abell 3526
A3526 alsoKnownAs Abell 3526