gptkbp:instance_of
|
gptkb:galaxy
|
gptkbp:bfsLayer
|
4
|
gptkbp:bfsParent
|
gptkb:Veigar
gptkb:Lockheed_Martin_C-5_M_Super_Galaxy
|
gptkbp:can_be
|
gptkb:football_club
Nebulae
Dark Matter Halo
Supernova Events
Multiple Nuclei
Stellar Winds
|
gptkbp:can_create
|
Star Clusters
|
gptkbp:contains
|
gptkb:Company
gptkb:Dust
Stars
|
gptkbp:exhibits
|
gptkb:Active_Galactic_Nuclei
Tidal Forces
Gravitational Lensing
Bar Structure
Starburst Activity
|
gptkbp:has_history
|
gptkb:launch_complex
|
gptkbp:hosts
|
Planets
Exoplanets
Star Formation Regions
|
https://www.w3.org/2000/01/rdf-schema#label
|
Super Galaxy
|
gptkbp:is_affected_by
|
gptkb:nebula
Cosmic Expansion
Cosmic Radiation
|
gptkbp:is_associated_with
|
Galaxy Mergers
|
gptkbp:is_characterized_by
|
Chemical Enrichment
Spiral Arms
High Luminosity
Dynamical Interactions
|
gptkbp:is_connected_to
|
Intergalactic Medium
Other Galaxies
Galaxy Evolution Models
|
gptkbp:is_described_as
|
Hubble's Law
|
gptkbp:is_found_in
|
Galaxy Catalogs
|
gptkbp:is_home_to
|
Various Stellar Populations
|
gptkbp:is_influenced_by
|
gptkb:Cosmic_Microwave_Background
|
gptkbp:is_observed_in
|
gptkb:physicist
Infrared Light
Radio Waves
Various Wavelengths
|
gptkbp:is_part_of
|
gptkb:fictional_universe
gptkb:star
Large Scale Structure
Cosmic Web
Galaxy Filaments
Galaxy Superclusters
|
gptkbp:is_studied_in
|
gptkb:observatory
Astronomers
Galaxy Evolution
Star Formation Rates
|
gptkbp:is_subject_to
|
Gravitational Forces
|
gptkbp:length
|
Large
|
gptkbp:located_in
|
Cosmic Structures
|
gptkbp:map
|
gptkb:Telescopes
|
gptkbp:mass
|
gptkb:High
|
gptkbp:scientific_classification
|
gptkb:Lenticular_Galaxy
Active Galaxy
|
gptkbp:type
|
gptkb:Spiral_Galaxy
|