Statements (55)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:can_be_formed_through |
dynamical interactions
|
| gptkbp:can_be_found_in |
gptkb:the_Local_Group
gptkb:elliptical_galaxies dwarf galaxies |
| gptkbp:can_contain |
multiple stellar populations
blue straggler stars |
| gptkbp:exhibits |
variable stars
|
| gptkbp:formed |
mergers of smaller clusters
|
| gptkbp:has_a_focus_on |
stellar dynamics research
|
| gptkbp:has_a_formation_history |
linked to galaxy formation
|
| gptkbp:hosts |
millisecond pulsars
|
| https://www.w3.org/2000/01/rdf-schema#label |
Type I globular cluster
|
| gptkbp:influence |
galactic evolution
|
| gptkbp:is_a_key_component_of |
galactic halos
|
| gptkbp:is_a_subject_of |
observational astronomy
|
| gptkbp:is_analyzed_in |
cosmological distances
|
| gptkbp:is_associated_with |
the formation of supermassive black holes
younger stars |
| gptkbp:is_characterized_by |
a high density of stars
a high star density a higher concentration of heavy elements a lack of gas and dust |
| gptkbp:is_different_from |
Type II globular cluster
|
| gptkbp:is_essential_for |
understanding dark matter
understanding stellar populations understanding galaxy dynamics |
| gptkbp:is_found_in |
galaxies
|
| gptkbp:is_observed_in |
gptkb:the_Milky_Way
gptkb:Hubble_Space_Telescope |
| gptkbp:is_often_associated_with |
galactic mergers
galactic bulges |
| gptkbp:is_often_compared_to |
gptkb:Type_II_globular_clusters
open star clusters |
| gptkbp:is_often_seen_in |
the center of galaxies
the outskirts of galaxies rich clusters of galaxies |
| gptkbp:is_often_used_in |
distance ladder methods
|
| gptkbp:is_part_of |
the halo of a galaxy
|
| gptkbp:is_recognized_by |
their color-magnitude diagrams
their luminosity functions |
| gptkbp:is_studied_for |
chemical evolution of galaxies
the formation of galaxies stellar populations |
| gptkbp:is_studied_in |
astrophysics
stellar evolution its gravitational interactions the age of the universe the cosmic microwave background. |
| gptkbp:is_typically_older_than |
open clusters
|
| gptkbp:metallicity |
high
|
| gptkbp:scientific_classification |
its metallicity and age
|
| gptkbp:type_of |
gptkb:star
|
| gptkbp:bfsParent |
gptkb:NGC_7078
|
| gptkbp:bfsLayer |
6
|