Luminous Infrared Galaxy

GPTKB entity

Statements (65)
Predicate Object
gptkbp:instance_of gptkb:galaxy
gptkbp:bfsLayer 5
gptkbp:bfsParent gptkb:NGC_253_L
gptkbp:can_be massive star clusters
gptkbp:exhibits complex morphology
strong emission lines
variability
outflows
gptkbp:has_luminosity 10^11 to 10^12 L☉
https://www.w3.org/2000/01/rdf-schema#label Luminous Infrared Galaxy
gptkbp:includes ULIR Gs
gptkbp:is_analyzed_in gptkb:musician
gptkb:nebula
computer simulations
the context of galaxy clusters
the context of galaxy formation
the context of galaxy interactions
the effects of environment on galaxy formation
gptkbp:is_associated_with supernovae
star formation
galaxy mergers
feedback processes
galaxy evolution theories
cosmic star formation history
gptkbp:is_characterized_by high metallicity
high infrared luminosity
high star formation rates
strong infrared emission
intense radiation fields
extensive star formation
high dust content
gptkbp:is_essential_for gptkb:spacecraft
gptkbp:is_explored_in the role of AGN
gptkbp:is_found_in merging galaxies
the infrared background
the local universe
gptkbp:is_influenced_by environmental factors
gptkbp:is_observed_in deep field surveys
gptkbp:is_often_compared_to normal galaxies
gptkbp:is_often_depicted_as infrared wavelengths
clusters of galaxies
high-redshift studies
the infrared luminosity function
gptkbp:is_part_of the cosmic web
the large-scale structure of the universe
the Hubble sequence
the IR galaxy population
gptkbp:is_recognized_by IRAS survey
gptkbp:is_related_to gptkb:active_galactic_nuclei
gptkb:quasars
molecular gas
the interstellar medium
stellar feedback
gptkbp:is_studied_in gptkb:observatory
galactic dynamics
multi-wavelength observations
chemical evolution
stellar populations
the formation of massive stars
galaxy evolution
the relationship between star formation and black holes
gptkbp:is_used_for dust obscuration
gptkbp:recognizes submillimeter telescopes
gptkbp:scientific_classification gptkb:galaxy
LIRG