|
gptkbp:instance_of
|
gptkb:astronomy
|
|
gptkbp:associated_with
|
gptkb:Large_Magellanic_Cloud
gptkb:Small_Magellanic_Cloud
|
|
gptkbp:components
|
the intergalactic medium
|
|
gptkbp:composed_of
|
gptkb:natural_gas
hydrogen gas
|
|
gptkbp:conducts_research_on
|
galactic evolution
|
|
gptkbp:contains
|
gptkb:interstellar_medium
hydrogen gas
|
|
gptkbp:discovered_by
|
gptkb:Harlow_Shapley
1970s
|
|
gptkbp:distance_from_earth
|
approximately 200,000 light-years
|
|
gptkbp:feature
|
the southern celestial hemisphere
the Local Group of galaxies
|
|
gptkbp:has_component
|
streaming gas
|
|
gptkbp:has_expansion
|
gptkb:the_Magellanic_Clouds
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Magellanic Stream
|
|
gptkbp:interacts_with
|
Milky Way's halo gas
|
|
gptkbp:investigates
|
galactic structure
|
|
gptkbp:is_a_feature_of_interest_for
|
galactic dynamics
|
|
gptkbp:is_a_feature_that_helps_explain
|
the distribution of dark matter in the Milky Way
|
|
gptkbp:is_a_source_of
|
the history of the Milky Way
metal-poor gas
|
|
gptkbp:is_a_subject_of
|
observational astronomy
astrophysical modeling
|
|
gptkbp:is_a_target_for_studies_on
|
galactic structure
|
|
gptkbp:is_affected_by
|
gptkb:dark_matter
galactic winds
|
|
gptkbp:is_analyzed_in
|
chemical composition
|
|
gptkbp:is_associated_with
|
gptkb:dark_matter
gptkb:Large_Magellanic_Cloud
gptkb:Small_Magellanic_Cloud
cosmic rays
star formation regions
star clusters
|
|
gptkbp:is_characterized_by
|
high-velocity clouds
|
|
gptkbp:is_connected_to
|
gptkb:the_Magellanic_Bridge
baryonic matter
galactic mergers
galactic rotation
galactic outflows
tidal interactions
|
|
gptkbp:is_considered
|
stellar formation theories
|
|
gptkbp:is_described_as
|
gptkb:literature
|
|
gptkbp:is_essential_for
|
galaxy formation
|
|
gptkbp:is_examined_in
|
gptkb:cosmology
magnetic fields
star formation history
|
|
gptkbp:is_explored_in
|
observational astronomy
|
|
gptkbp:is_influenced_by
|
supernovae
cosmic rays
gravitational interactions
|
|
gptkbp:is_linked_to
|
the evolution of the Milky Way
|
|
gptkbp:is_located_in
|
the southern sky
|
|
gptkbp:is_observed_in
|
gptkb:astronomy
radio telescopes
radio wavelengths
infrared wavelengths
multiple wavelengths
HI 21 cm emission
|
|
gptkbp:is_part_of
|
gptkb:Local_Group
gptkb:Milky_Way_Galaxy
Milky Way's structure
large-scale structure
intergalactic medium
cosmic web
galactic filaments
|
|
gptkbp:is_part_of_a_larger_phenomenon
|
galactic interactions
|
|
gptkbp:is_part_of_a_larger_structure
|
Magellanic System
|
|
gptkbp:is_related_to
|
galactic evolution
stellar populations
galactic interactions
|
|
gptkbp:is_said_to_be
|
a remnant of past interactions
|
|
gptkbp:is_significant_for
|
understanding the Local Group's dynamics
|
|
gptkbp:is_studied_for
|
gptkb:dark_matter
cosmic evolution
|
|
gptkbp:is_studied_in
|
gptkb:cosmology
astrophysics
computer simulations
|
|
gptkbp:is_thought_to_originate_from
|
gptkb:the_Magellanic_Clouds
|
|
gptkbp:is_visible_from
|
gptkb:Earth
|
|
gptkbp:key_feature
|
understanding galaxy mergers
|
|
gptkbp:length
|
approximately 1.3 million light-years
approximately 75,000 light-years
|
|
gptkbp:located_in
|
gptkb:Milky_Way_Galaxy
|
|
gptkbp:map
|
radio telescopes
galactic surveys
3 D space
|
|
gptkbp:originated_in
|
gptkb:Magellanic_Clouds
|
|
gptkbp:part_of
|
gptkb:Ring_of_Honor
|
|
gptkbp:preserved_by
|
the Magellanic Clouds' interaction with the Milky Way
|
|
gptkbp:research_focus
|
galactic winds
|
|
gptkbp:significance
|
galactic dynamics
|
|
gptkbp:structure
|
the study of galaxy interactions
|
|
gptkbp:targets
|
future astronomical surveys
|
|
gptkbp:type_of
|
tidal stream
|
|
gptkbp:bfsParent
|
gptkb:Magellanic_cloud
gptkb:LMC_(Large_Magellanic_Cloud)
gptkb:Large_Magellanic_Cloud
gptkb:Small_Magellanic_Cloud
|
|
gptkbp:bfsLayer
|
6
|