Pavo–Indus filament
E511403
The Pavo–Indus filament is a massive, elongated large-scale structure of galaxies forming part of the cosmic web in the nearby universe.
Statements (29)
| Predicate | Object |
|---|---|
| instanceOf |
galaxy filament
ⓘ
large-scale structure of the universe ⓘ |
| contains |
galaxies
ⓘ
galaxy clusters ⓘ galaxy groups ⓘ |
| hasComponent |
baryonic matter
ⓘ
dark matter ⓘ intergalactic medium ⓘ |
| hasDynamics | influenced by gravity ⓘ |
| hasEnvironment | low-redshift universe ⓘ |
| hasMass | massive ⓘ |
| hasRedshiftRange | low redshift ⓘ |
| hasRole |
connects galaxy clusters
ⓘ
traces matter distribution on large scales ⓘ |
| hasShape | elongated ⓘ |
| hasSignificance |
constrains models of structure formation
ⓘ
traces dark matter distribution ⓘ |
| hasSpatialScale | tens to hundreds of megaparsecs ⓘ |
| hasStructureType | anisotropic ⓘ |
| locatedIn | nearby universe ⓘ |
| namedAfter |
Indus constellation
NERFINISHED
ⓘ
Pavo constellation NERFINISHED ⓘ |
| observedIn |
X-ray wavelengths
ⓘ
optical wavelengths ⓘ radio wavelengths ⓘ |
| partOf | cosmic web ⓘ |
| studiedInField |
extragalactic astronomy
ⓘ
large-scale structure of the cosmos ⓘ observational cosmology ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.