NGC 4696

E610635

NGC 4696 is a massive elliptical galaxy that serves as the central dominant galaxy of the Centaurus Cluster, notable for its complex dust lanes and active galactic nucleus.

Jump to: Surface forms Statements Referenced by

Observed surface forms (1)

Surface form Occurrences
NGC 4696A 1

Statements (45)

Predicate Object
instanceOf central dominant galaxy
elliptical galaxy
radio galaxy
angularSize ~4.5 × 3.5 arcminutes
apparentMagnitudeV ~11.4
catalog New General Catalogue NERFINISHED
declination −41° 18′ 40″ (J2000)
discoveredBy John Herschel NERFINISHED
discoveryDate 1834
distanceFromEarth ~150 million light-years
~46 Mpc
environment rich galaxy cluster core
hasActiveGalacticNucleus true
hasAGNFeedbackOnIntraclusterMedium true
hasAlternativeName 2MASX J12484980-4118394 NERFINISHED
ESO 322- G 091 NERFINISHED
PKS 1246-410 NERFINISHED
hasCentralCoolingFlowFeatures true
hasComplexDustStructure true
hasComplexIonizedGasFilaments true
hasCoolCoreClusterEnvironment true
hasDustLanes true
hasExtendedHalo true
hasFilamentaryDustLanes true
hasIntraclusterLightContribution significant
hasJetActivity true
hasMorphologicalType E
hasOpticalEmissionLineFilaments true
hasRadioSourceDesignation PKS 1246-41 NERFINISHED
hasStellarPopulation predominantly old stars
hasSupermassiveBlackHole true
hasXRayEmission true
hostClusterAlternativeName Abell 3526 NERFINISHED
isBrightestClusterGalaxy true
isCentralGalaxyOf Centaurus Cluster NERFINISHED
isDominantGalaxyInRegion Centaurus Cluster core NERFINISHED
locatedInConstellation Centaurus NERFINISHED
memberOf Centaurus Cluster NERFINISHED
observedInRadioBy VLA NERFINISHED
observedInXRayBy Chandra X-ray Observatory NERFINISHED
XMM-Newton NERFINISHED
radialVelocity ~2970 km/s
redshift 0.0099
rightAscension 12h 48m 49s (J2000)
showsEvidenceOf past merger events

Referenced by (4)

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

Centaurus Cluster containsGalaxy NGC 4696
this entity surface form: NGC 4696A