Abell 2597

E465456

Abell 2597 is a distant galaxy cluster notable for its central active galaxy and cooling-flow features, observed extensively in X-ray and radio wavelengths.

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Statements (47)

Predicate Object
instanceOf Abell galaxy cluster
galaxy cluster
catalogCode A2597 NERFINISHED
discoveredBy George O. Abell (via Abell cluster catalog) NERFINISHED
hasActiveGalacticNucleus yes
hasCentralBlackHole supermassive black hole
hasCentralGalaxy Abell 2597 Brightest Cluster Galaxy NERFINISHED
BCG in Abell 2597 NERFINISHED
hasCoolingFlow yes
hasDistanceFromEarth on the order of hundreds of megaparsecs
hasEnvironment dense intracluster medium
hasFeature AGN feedback
X-ray bright core
X-ray cavities
cold gas filaments
cooling-flow cluster core
molecular gas in cluster core
multiphase intracluster medium
optical emission-line nebula
radio jets from central AGN
radio lobes
hasObservationType deep X-ray imaging
infrared observations
optical spectroscopy
radio interferometry
hasPhysicalProcess AGN heating of intracluster medium
cooling-flow induced star formation
jet–ICM interaction
radiative cooling of intracluster gas
hasRedshift approximately 0.085
locatedIn constellation Aquarius NERFINISHED
memberOf nearby rich galaxy clusters at z~0.1
observedByTelescope Chandra X-ray Observatory NERFINISHED
Hubble Space Telescope NERFINISHED
Very Large Array NERFINISHED
XMM-Newton NERFINISHED
observedInWavelength X-ray
optical
radio
partOf Abell catalog of rich clusters of galaxies NERFINISHED
showsPhenomenon X-ray surface brightness peak at cluster center
central temperature drop in intracluster gas
radio bubbles coincident with X-ray cavities
star formation in brightest cluster galaxy
usedAsExampleOf AGN feedback in clusters
cool-core galaxy cluster
cooling-flow problem studies

Referenced by (2)

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