gptkbp:instance_of
|
gptkb:galaxy
|
gptkbp:are_a_key_area_for
|
observational astronomy.
|
gptkbp:are_a_satellite_of
|
gptkb:the_Milky_Way
|
gptkbp:are_a_source_of_interest_for
|
extragalactic astronomy
|
gptkbp:are_important_for_studying
|
galactic evolution
stellar populations
|
gptkbp:are_irregular_galaxies
|
gptkb:true
nan
|
gptkbp:are_irregular_in_shape
|
nan
|
gptkbp:are_known_for
|
gptkb:supernova_remnants
variable stars
H II regions
star clusters
their unique properties
their star formation history
their irregular shapes
their irregular structure
|
gptkbp:are_located_at_a_distance_of
|
approximately 163,000 light-years from Earth
|
gptkbp:are_located_in_the_constellation
|
gptkb:Doradus
|
gptkbp:are_often_included_in_studies_of
|
galaxy mergers
|
gptkbp:are_often_used_to_study
|
stellar evolution
|
gptkbp:are_often_used_to_test
|
cosmological models
|
gptkbp:are_part_of
|
the Local Group of galaxies
the Magellanic Stream
the Magellanic System
LMC-SMC system
Magellanic System
LMC and SMC
|
gptkbp:are_thought_to_have_formed
|
from the same primordial gas as the Milky Way
|
gptkbp:are_thought_to_have_interacted_with
|
the Milky Way in the past
|
gptkbp:are_visible_to_the_naked_eye
|
nan
|
gptkbp:contains
|
gptkb:Large_Magellanic_Cloud
gptkb:Small_Magellanic_Cloud
young stars
old stars
|
gptkbp:discovered_by
|
gptkb:Ferdinand_Magellan
|
gptkbp:has_supernova
|
gptkb:true
|
gptkbp:have_a_significant_amount_of
|
gptkb:dark_matter
|
gptkbp:have_been_mapped_by
|
gptkb:astronomy
|
gptkbp:have_been_mapped_in_detail_by
|
various astronomical surveys
|
gptkbp:have_different_morphologies
|
gptkb:true
|
gptkbp:have_dwarf_galaxies
|
gptkb:true
|
gptkbp:have_galactic_interactions
|
gptkb:true
|
gptkbp:have_multiple_star_clusters
|
gptkb:true
|
gptkbp:have_star_clusters
|
gptkb:true
|
gptkbp:have_star_formation_regions
|
gptkb:true
|
https://www.w3.org/2000/01/rdf-schema#label
|
the Magellanic Clouds
|
gptkbp:include
|
gptkb:the_Large_Magellanic_Cloud
gptkb:the_Small_Magellanic_Cloud
|
gptkbp:interacts_with
|
gptkb:Milky_Way
|
gptkbp:is_a_key_component_of
|
the Local Group's dynamics
|
gptkbp:is_a_source_of
|
cosmic rays
stellar feedback research
|
gptkbp:is_a_subject_of
|
astrophysicists
galactic archaeology
|
gptkbp:is_approximately
|
163,000 light-years away from Earth
|
gptkbp:is_associated_with
|
gptkb:dark_matter
gptkb:the_Magellanic_Bridge
star formation regions
the Magellanic Stream
|
gptkbp:is_considered
|
satellite galaxies of the Milky Way
|
gptkbp:is_essential_for
|
cosmic evolution
|
gptkbp:is_home_to
|
young stars
H II regions
star-forming regions
old stars
nebulae
massive stars
the Tarantula Nebula
|
gptkbp:is_involved_in
|
galactic dynamics
intergalactic interactions
|
gptkbp:is_located_in
|
gptkb:the_Local_Group
the southern celestial hemisphere
the constellation Dorado
the constellation Mensa
|
gptkbp:is_located_near
|
gptkb:the_Milky_Way
gptkb:South_Celestial_Pole
gptkb:the_Milky_Way_Galaxy
|
gptkbp:is_observed_in
|
gptkb:Hubble_Space_Telescope
|
gptkbp:is_often_compared_to
|
gptkb:the_Andromeda_Galaxy
other irregular galaxies
|
gptkbp:is_often_depicted_as
|
star charts
|
gptkbp:is_often_discussed_in
|
dark matter distribution
|
gptkbp:is_often_referenced_in
|
astronomical literature
distance measurement in astronomy
|
gptkbp:is_often_seen_in
|
infrared wavelengths
|
gptkbp:is_part_of
|
gptkb:Local_Group
|
gptkbp:is_studied_for
|
chemical composition
stellar evolution
star formation history
their chemical composition
their dynamics
their interaction with the Milky Way
|
gptkbp:is_studied_in
|
gptkb:astronomy
the Milky Way's structure
galactic winds
|
gptkbp:is_used_in
|
cosmological studies
|
gptkbp:is_visible_from
|
gptkb:Earth
gptkb:the_Earth
the naked eye
the Southern Hemisphere
the night sky
northern and southern hemispheres
the southern sky
|
gptkbp:located_in
|
Southern Hemisphere
|
gptkbp:named_after
|
gptkb:Ferdinand_Magellan
|
gptkbp:research_focus
|
gptkb:cosmology
|
gptkbp:targets
|
future astronomical missions
|
gptkbp:bfsParent
|
gptkb:the_Milky_Way_galaxy
|
gptkbp:bfsLayer
|
4
|