Statements (66)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
Galaxy
|
| gptkbp:contains |
Old stars
|
| gptkbp:has |
Significant amounts of gas and dust
|
| gptkbp:hasFacilities |
Greater than 10^11 solar masses
|
| gptkbp:hasType |
gptkb:Elliptical_Galaxy
|
| https://www.w3.org/2000/01/rdf-schema#label |
Giant Elliptical Galaxy
|
| gptkbp:isAccessibleBy |
gptkb:Earth
|
| gptkbp:isAssociatedWith |
Dark matter
Active galactic nuclei Galaxy mergers Galaxy cluster dynamics Galaxy clusters formation Galaxy evolution models Galaxy formation history |
| gptkbp:isCharacterizedBy |
Low metallicity
High density of stars Smooth light profile Elliptical shape High stellar density Lack of spiral structure Low angular momentum |
| gptkbp:isFoundIn |
gptkb:Coma_Cluster
gptkb:Abell_168 gptkb:Abell_85 Galaxy clusters Abell 2744 Abell_2029 Perseus_Cluster |
| gptkbp:isHomeTo |
Globular clusters
|
| gptkbp:isInformedBy |
Merging of smaller galaxies
|
| gptkbp:isKnownFor |
Interstellar medium
Bright central regions Low star formation rate Multiple stellar populations Presence of dark matter halos Presence of supernova remnants X-ray emitting gas |
| gptkbp:isLocatedIn |
Galaxy superclusters
|
| gptkbp:isOftenMadeWith |
Irregular galaxies
Dwarf elliptical galaxies Lenticular galaxies |
| gptkbp:isOftenUsedIn |
Cosmology
Astronomical research Observational astronomy Astrophysical simulations Rich galaxy clusters |
| gptkbp:isPartOf |
Large-scale structure of the universe
Galaxy formation theories Cosmic web Galaxy classification schemes Galaxy evolution studies Large-scale galaxy surveys |
| gptkbp:isRelatedTo |
Supermassive black holes
|
| gptkbp:isServedBy |
Radio telescopes
Infrared_wavelengths |
| gptkbp:isSetIn |
Spiral Galaxy
|
| gptkbp:isStudiedIn |
Astrophysics
Galaxy evolution Galaxy interactions Galaxy morphology Stellar population analysis Galaxy dynamics Galaxy cluster evolution. |
| gptkbp:isUsedFor |
gptkb:Virgo_Cluster
Hubble classification system |
| gptkbp:resolution |
High luminosity
|