Statements (59)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:galaxy
|
gptkbp:bfsLayer |
3
|
gptkbp:bfsParent |
gptkb:nebula
|
gptkbp:can_be |
gptkb:active_galactic_nuclei
high metallicity high surface brightness complex morphologies multiple star formation episodes |
gptkbp:can_lead_to |
formation of globular clusters
|
gptkbp:exhibits |
intense radiation
variability in brightness dust lanes outflows of gas extreme stellar winds high levels of ionization |
gptkbp:formed |
gas-rich mergers
|
https://www.w3.org/2000/01/rdf-schema#label |
Starburst galaxies
|
gptkbp:influence |
galactic winds
galaxy morphology their surrounding environment |
gptkbp:is_associated_with |
supernovae
|
gptkbp:is_characterized_by |
high star formation rate
|
gptkbp:is_considered |
important for star formation theories
|
gptkbp:is_essential_for |
understanding galaxy evolution
understanding the universe's expansion galactic ecology |
gptkbp:is_found_in |
galaxy clusters
the infrared background the local universe |
gptkbp:is_known_for |
produce heavy elements
|
gptkbp:is_observed_in |
infrared wavelengths
|
gptkbp:is_often_associated_with |
cosmic rays
high luminosity stellar nurseries massive stars starburst regions |
gptkbp:is_often_compared_to |
normal galaxies
young galaxies |
gptkbp:is_often_depicted_as |
the early universe
interacting galaxy pairs the outskirts of galaxy clusters |
gptkbp:is_often_used_in |
cosmological simulations
|
gptkbp:is_recognized_by |
their spectral lines
their emission lines |
gptkbp:is_related_to |
gptkb:quasars
|
gptkbp:is_studied_in |
gptkb:musician
gptkb:Hubble_Space_Telescope astrophysics the context of galaxy formation the context of dark energy. their chemical evolution their impact on galaxy interactions |
gptkbp:key |
understanding cosmic evolution
understanding dark matter |
gptkbp:recognizes |
radio telescopes
|
gptkbp:scientific_classification |
their luminosity
ultra-luminous infrared galaxies star-forming galaxies their star formation history |