Statements (56)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:observatory
|
| gptkbp:associated_with |
Galaxy formation
Galaxy clusters Chemical_evolution_of_galaxies |
| gptkbp:contains |
Dark matter
Old stars Globular clusters Primordial gas |
| gptkbp:expansion |
Far beyond the visible galaxy
|
| gptkbp:features |
Observational astronomy
Elliptical galaxies |
| gptkbp:formed |
From early galaxy interactions
|
| gptkbp:has_a |
Complex formation history
|
| gptkbp:has_a_focus_on |
Cosmology
Astrophysical research |
| gptkbp:hosts |
Dark matter halos
|
| https://www.w3.org/2000/01/rdf-schema#label |
Galactic Halo
|
| gptkbp:impact |
Stellar orbits
|
| gptkbp:includes |
Baryonic_matter
|
| gptkbp:influence |
Star formation rates
|
| gptkbp:influenced |
Galaxy mergers
|
| gptkbp:is_a_key_component_of |
Milky Way
Galaxy assembly processes Luminous matter |
| gptkbp:is_a_model_for |
A dark matter-dominated region
|
| gptkbp:is_a_source_of |
Cosmic rays
|
| gptkbp:is_a_subject_of |
Galaxy interactions
Galactic archaeology Theoretical astrophysics Extragalactic astronomy |
| gptkbp:is_available_in |
Spiral galaxies
|
| gptkbp:is_characterized_by |
Low density
|
| gptkbp:is_essential_for |
Understanding galaxy evolution
|
| gptkbp:is_featured_in |
Astronomical models
A spheroidal structure |
| gptkbp:is_involved_in |
Galaxy dynamics
|
| gptkbp:is_linked_to |
Cosmological simulations
|
| gptkbp:is_part_of |
Galaxy
|
| gptkbp:is_studied_in |
Astrophysics
Spectroscopy Gravitational lensing |
| gptkbp:is_used_in |
N-body simulations
Other galactic halos |
| gptkbp:region |
Space
Mapped in three dimensions Probed by gravitational waves Star clusters can be found Stellar populations can be studied Studied through simulations. |
| gptkbp:related_to |
Astrobiology
Galaxy rotation curves |
| gptkbp:shape |
Galactic_winds
|
| gptkbp:surroundingArea |
Galactic_disk
|
| gptkbp:visitedBy |
X-ray observations
Galaxy surveys |
| gptkbp:waterQuality |
Galactic_disk
|