Statements (65)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:astronomy
|
| gptkbp:affects |
galactic dynamics
|
| gptkbp:are_measured_by |
redshift
|
| gptkbp:are_often_mapped_by |
surveys
|
| gptkbp:are_part_of |
large-scale structure of the universe
|
| gptkbp:are_typically_formed_by |
merging smaller clusters
|
| gptkbp:bounded_by |
gravity
|
| gptkbp:can |
hot gas
central galaxies subclusters |
| gptkbp:can_be_found_in |
various wavelengths
|
| gptkbp:can_be_mapped_using |
gravitational wave observations
|
| gptkbp:can_contain |
gptkb:dark_matter
thousands of galaxies intracluster medium |
| gptkbp:can_detect |
X-ray observations
|
| gptkbp:consists_of |
galaxies
|
| gptkbp:exhibits |
X-ray emissions
gravitational lensing temperature gradients merging activity |
| https://www.w3.org/2000/01/rdf-schema#label |
Galaxy Clusters
|
| gptkbp:influence |
the cosmic microwave background
galaxy evolution |
| gptkbp:is_a_key_component_of |
the cosmic web
|
| gptkbp:is_analyzed_in |
gptkb:spectroscopy
cosmological simulations the nature of dark energy their gravitational potential their velocity dispersion |
| gptkbp:is_associated_with |
baryonic matter
cosmic microwave background radiation galactic clusters |
| gptkbp:is_characterized_by |
temperature
|
| gptkbp:is_essential_for |
studying dark energy
testing general relativity understanding galaxy interactions understanding cosmic structure |
| gptkbp:is_explored_in |
the history of the universe
|
| gptkbp:is_found_in |
the universe
|
| gptkbp:is_linked_to |
supernovae
|
| gptkbp:is_observed_in |
infrared wavelengths
|
| gptkbp:is_often_associated_with |
gptkb:active_galactic_nuclei
|
| gptkbp:is_often_seen_in |
filaments of dark matter
|
| gptkbp:is_often_used_in |
astrophysics research
astrophysical modeling |
| gptkbp:is_recognized_by |
their luminosity
their X-ray brightness |
| gptkbp:is_studied_for |
the role of dark matter
their mass distribution |
| gptkbp:is_studied_in |
gptkb:astronomy
multi-wavelength observations simulations radio telescopes large-scale structure formation |
| gptkbp:is_tested_for |
cosmological models
|
| gptkbp:key |
the evolution of the universe
the universe's expansion the distribution of matter in the universe |
| gptkbp:provides_information_on |
galaxy formation
|
| gptkbp:scientific_classification |
morphology
rich or poor clusters their density profile |
| gptkbp:bfsParent |
gptkb:Hubble_Space_Telescope
|
| gptkbp:bfsLayer |
4
|