Properties (55)
Predicate | Object |
---|---|
gptkbp:instanceOf |
galactic structure
|
gptkbp:associated_with |
the interstellar medium
|
gptkbp:composedOf |
young stars
|
gptkbp:contains |
gas
dust stars stellar nurseries open clusters |
gptkbp:has_a |
about 1,000 light-years
about 15,000 light-years |
gptkbp:has_a_focus_on |
cosmological simulations
galactic evolution studies galactic_archaeology |
https://www.w3.org/2000/01/rdf-schema#label |
Milky Way's thin disk
|
gptkbp:impact |
galactic dynamics
|
gptkbp:influenced |
dark matter
galactic winds the galactic bulge |
gptkbp:is_a_key_component_of |
the Milky Way's disk
|
gptkbp:is_a_site_for |
supernova remnants
chemical enrichment planetary system formation |
gptkbp:is_characterized_by |
spiral arms
a diverse range of stellar types a flat geometry a high concentration of young stars a high density of stars a high rate of supernovae a variety of stellar populations |
gptkbp:is_home_to |
the majority of the galaxy's stars
|
gptkbp:is_involved_in |
galactic interactions
galactic rotation |
gptkbp:is_located_in |
the galactic plane
massive stars evolve most star formation occurs the solar system is located the_Galactic_Center_is_located the_Orion_Arm_is_located the_Sun_orbits |
gptkbp:is_part_of |
Milky Way galaxy
the galactic disk the Milky Way's structure the Milky Way's spiral structure the larger galactic structure the_Milky_Way's_overall_mass_distribution |
gptkbp:is_studied_in |
astrophysics
radio telescopes its star formation history stellar population surveys |
gptkbp:region |
high metallicity
active star formation stellar density gradients stellar migration |
gptkbp:surroundedBy |
the galactic halo
|
gptkbp:visitedBy |
optical wavelengths
|