Starburst Galaxies

GPTKB entity

Statements (58)
Predicate Object
gptkbp:instance_of gptkb:galaxy
gptkbp:associated_with gptkb:active_galactic_nuclei
gptkbp:can massive star clusters
gptkbp:can_be_found_in galaxy clusters
the early universe
the local universe
gptkbp:can_contain supernovae
gptkbp:can_lead_to gas inflow
formation of new stars
gptkbp:characterized_by high star formation rate
gptkbp:exhibits intense radiation
variability in brightness
stellar population gradients
dust obscuration
outflows of gas
different star formation histories
variations in star formation rates
gptkbp:has_a_focus_on astronomical surveys
theoretical models.
gptkbp:has_influence_on galactic evolution
https://www.w3.org/2000/01/rdf-schema#label Starburst Galaxies
gptkbp:is_analyzed_in gptkb:spectroscopy
computer simulations
the context of dark matter
gptkbp:is_associated_with stellar feedback processes
gptkbp:is_essential_for understanding dark energy
understanding galaxy evolution
star formation theories
the study of galaxy interactions
gptkbp:is_found_in various redshift ranges
gptkbp:is_observed_in space telescopes
infrared wavelengths
gptkbp:is_often_associated_with high-energy phenomena
cosmic reionization
molecular gas clouds
gptkbp:is_often_compared_to gptkb:quasars
short-lived phenomena
the result of galaxy mergers
more luminous than normal galaxies
gptkbp:is_often_described_as high metallicity
gptkbp:is_often_seen_in interacting galaxy pairs
gptkbp:is_often_used_in simulations of cosmic evolution
gptkbp:is_recognized_by their spectral lines
their morphology
their emission lines
gptkbp:is_studied_for their chemical composition
gptkbp:is_studied_in astrophysics
multi-wavelength observations
X-ray observations
radio observations
the context of galaxy formation
gptkbp:key cosmological studies
understanding cosmic structure formation
gptkbp:scientific_classification their luminosity
ultra-luminous infrared galaxies
star-forming galaxies
gptkbp:bfsParent gptkb:Hubble_Space_Telescope
gptkbp:bfsLayer 4