Abell 262
E553750
Abell 262 is a nearby galaxy cluster in the constellation Andromeda, notable for its relatively low mass and cool-core intracluster medium within the Perseus–Pisces Supercluster.
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
Abell galaxy cluster
ⓘ
extragalactic astronomical object ⓘ galaxy cluster ⓘ |
| cataloguedIn | Abell catalogue of rich clusters of galaxies NERFINISHED ⓘ |
| containsGalaxy |
NGC 703
NERFINISHED
ⓘ
NGC 704 NERFINISHED ⓘ NGC 705 NERFINISHED ⓘ NGC 709 NERFINISHED ⓘ NGC 710 NERFINISHED ⓘ UGC 130 NERFINISHED ⓘ |
| distanceFromEarth |
approximately 200 million light-years
ⓘ
approximately 60 Mpc ⓘ |
| environment | relatively low-density large-scale environment ⓘ |
| hasAlternativeName |
ACO 262
NERFINISHED
ⓘ
Abell Cluster 262 NERFINISHED ⓘ RXC J0152.0+3609 NERFINISHED ⓘ ZwCl 0144.4+3602 NERFINISHED ⓘ |
| hasBrightestClusterGalaxy | NGC 708 NERFINISHED ⓘ |
| hasCentralRadioSource | radio source associated with NGC 708 ⓘ |
| hasCoolingFlow | cooling flow in intracluster medium ⓘ |
| hasDeclination | +36° 09′ ⓘ |
| hasDynamicalState | relaxed core ⓘ |
| hasGalaxyPopulation | dominantly early-type galaxies ⓘ |
| hasGasTemperature | cooler core gas compared to outer regions ⓘ |
| hasGravitationalPotential | dominated by dark matter ⓘ |
| hasIntraclusterMediumType | cool-core intracluster medium ⓘ |
| hasMass | relatively low mass for a galaxy cluster ⓘ |
| hasMetallicityGradient | enhanced metallicity in cluster core ⓘ |
| hasMorphologicalType | poor cluster ⓘ |
| hasRedshift | 0.0163 ⓘ |
| hasRightAscension | 01h 52m ⓘ |
| hasSubstructure | evidence of subclusters and galaxy groups ⓘ |
| hasVelocityDispersion | relatively low velocity dispersion ⓘ |
| hasXRayEmission | extended X-ray emitting intracluster gas ⓘ |
| hasXRayLuminosity | low X-ray luminosity compared to rich clusters ⓘ |
| locatedInConstellation | Andromeda NERFINISHED ⓘ |
| memberOf | local universe ⓘ |
| observedInWavelength |
X-ray
ⓘ
optical ⓘ radio ⓘ |
| partOf | Perseus–Pisces Supercluster NERFINISHED ⓘ |
| studiedBy |
Chandra X-ray Observatory
NERFINISHED
ⓘ
ROSAT NERFINISHED ⓘ XMM-Newton NERFINISHED ⓘ |
| studiedFor |
AGN feedback in clusters
ⓘ
cool-core cluster physics ⓘ intracluster medium cooling and heating balance ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.