gptkbp:instance_of
|
gptkb:spiral_galaxy
|
gptkbp:can
|
multiple star clusters
high star density regions
|
gptkbp:can_be_found_in
|
gptkb:the_Local_Group
galaxy clusters
various cosmic environments
|
gptkbp:can_be_used_to
|
irregular star distribution
|
gptkbp:can_contain
|
gptkb:dark_matter
young stars
old stars
|
gptkbp:characteristic
|
lacks a distinct shape
|
gptkbp:contains
|
gptkb:natural_gas
dust
stars
|
gptkbp:exhibits
|
varied metallicity
|
gptkbp:hosts
|
gptkb:supernova_remnants
|
https://www.w3.org/2000/01/rdf-schema#label
|
Irr
|
gptkbp:is_a_key_component_of
|
galactic classification systems
|
gptkbp:is_a_subject_of
|
gptkb:cosmology
astrophysics research
|
gptkbp:is_affected_by
|
environmental factors
|
gptkbp:is_an_important_subject_in
|
galactic evolution studies
|
gptkbp:is_characterized_by
|
irregular morphology
|
gptkbp:is_different_from
|
gptkb:elliptical_galaxies
spiral galaxies
|
gptkbp:is_essential_for
|
galaxy formation processes
the diversity of galaxy types
|
gptkbp:is_found_in
|
various redshift ranges
|
gptkbp:is_influenced_by
|
gravitational interactions
|
gptkbp:is_observed_in
|
telescopes
different wavelengths
|
gptkbp:is_often_associated_with
|
gptkb:active_galactic_nuclei
star formation
|
gptkbp:is_often_compared_to
|
dwarf galaxies
|
gptkbp:is_often_described_as
|
irregularly shaped galaxy
|
gptkbp:is_often_seen_in
|
intergalactic space
low-density regions of space
other galaxy types
|
gptkbp:is_part_of
|
the universe
galaxy mergers
|
gptkbp:is_studied_in
|
gptkb:spectroscopy
gptkb:astronomy
its star formation history
|
gptkbp:may_have
|
active star formation regions
irregular gas clouds
|
gptkbp:may_show
|
signs of tidal interactions
|
gptkbp:may_show_signs_of
|
merging with other galaxies
|
gptkbp:often_includes
|
galaxy surveys
|
gptkbp:research_focus
|
galaxy dynamics
|
gptkbp:scientific_classification
|
Hubble classification system
a galaxy type
blue compact galaxies
|
gptkbp:type
|
gptkb:galaxy
|
gptkbp:type_of
|
non-spiral galaxy
|
gptkbp:bfsParent
|
gptkb:M82
|
gptkbp:bfsLayer
|
5
|