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.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Abell 262 canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T5846077 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: Abell 262 Context triple: [Perseus–Pisces Supercluster, contains, Abell 262]
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A.
Abell 3526
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.
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B.
Abell 3627
Abell 3627 is a massive, nearby galaxy cluster located in the direction of the Great Attractor region and is one of the most prominent components of the Hydra–Centaurus Supercluster.
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C.
Abell 1526
Abell 1526 is a galaxy cluster listed in the Abell catalog and associated with the larger Virgo Cluster region of galaxy clusters.
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D.
Abell 426
Abell 426, also known as the Perseus Cluster, is a massive, nearby galaxy cluster notable for its bright X-ray emission and central active galaxy NGC 1275.
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E.
Abell 1060
Abell 1060 is a nearby, rich galaxy cluster in the constellation Hydra, notable for its dense concentration of galaxies and role in studies of large-scale cosmic structure.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Abell 262 Target entity description: 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.
-
A.
Abell 3526
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.
-
B.
Abell 3627
Abell 3627 is a massive, nearby galaxy cluster located in the direction of the Great Attractor region and is one of the most prominent components of the Hydra–Centaurus Supercluster.
-
C.
Abell 1526
Abell 1526 is a galaxy cluster listed in the Abell catalog and associated with the larger Virgo Cluster region of galaxy clusters.
-
D.
Abell 426
Abell 426, also known as the Perseus Cluster, is a massive, nearby galaxy cluster notable for its bright X-ray emission and central active galaxy NGC 1275.
-
E.
Abell 1060
Abell 1060 is a nearby, rich galaxy cluster in the constellation Hydra, notable for its dense concentration of galaxies and role in studies of large-scale cosmic structure.
- F. None of above. chosen
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 ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Subject: Abell 262 Description of subject: 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.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.