Statements (99)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:observatory
|
| gptkbp:bfsLayer |
4
|
| gptkbp:bfsParent |
gptkb:Large_Magellanic_Cloud
gptkb:Small_Magellanic_Cloud |
| gptkbp:analyzes |
galactic structure
|
| gptkbp:associated_with |
gptkb:Large_Magellanic_Cloud
gptkb:Small_Magellanic_Cloud |
| gptkbp:composed_of |
gptkb:Company
hydrogen gas |
| gptkbp:conservation_efforts |
the Magellanic Clouds' interaction with the Milky Way
|
| gptkbp:contains |
gptkb:interstellar_medium
hydrogen gas |
| gptkbp:depicted_in |
gptkb:physicist
|
| gptkbp:discovered_by |
gptkb:Harlow_Shapley
1970s |
| gptkbp:distance |
approximately 200,000 light-years
|
| gptkbp:examines |
gptkb:spacecraft
magnetic fields star formation history |
| gptkbp:features |
the southern celestial hemisphere
the Local Group of galaxies the distribution of dark matter in the Milky Way |
| gptkbp:game_components |
the intergalactic medium
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:is_a_source_of |
the history of the Milky Way
metal-poor gas |
| gptkbp:is_affected_by |
gptkb:nebula
galactic winds |
| gptkbp:is_analyzed_in |
chemical composition
|
| gptkbp:is_associated_with |
gptkb:nebula
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:literary_work
|
| gptkbp:is_essential_for |
galaxy formation
|
| 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_observed_in |
gptkb:observatory
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_related_to |
galactic evolution
stellar populations galactic interactions |
| gptkbp:is_said_to_have |
a remnant of past interactions
|
| gptkbp:is_studied_in |
gptkb:spacecraft
gptkb:Monarch astrophysics computer simulations cosmic evolution |
| gptkbp:key |
understanding galaxy mergers
|
| gptkbp:length |
approximately 1.3 million light-years
approximately 75,000 light-years |
| gptkbp:located_in |
gptkb:Milky_Way_Galaxy
the southern sky |
| gptkbp:map |
radio telescopes
galactic surveys 3 D space |
| gptkbp:notable_feature |
galactic dynamics
understanding the Local Group's dynamics |
| gptkbp:origin |
gptkb:Magellanic_Clouds
gptkb:the_Magellanic_Clouds |
| gptkbp:part_of |
gptkb:item
|
| gptkbp:related_concept |
galactic interactions
|
| gptkbp:research |
galactic evolution
|
| gptkbp:research_focus |
galactic structure
galactic winds |
| gptkbp:significance |
galactic dynamics
|
| gptkbp:social_structure |
the study of galaxy interactions
Magellanic System |
| gptkbp:subject |
observational astronomy
astrophysical modeling |
| gptkbp:targets |
future astronomical surveys
|
| gptkbp:type_of |
tidal stream
|