|
gptkbp:instance_of
|
gptkb:star
|
|
gptkbp:are_difficult_to_observe
|
due to their distance
|
|
gptkbp:are_hypothesized_to_have
|
different evolutionary paths
short lifespans
|
|
gptkbp:are_part_of
|
stellar evolution theory
|
|
gptkbp:are_theoretical_objects
|
in astrophysics
|
|
gptkbp:are_thought_to_have
|
formed in clusters
|
|
gptkbp:consists_of
|
gptkb:hydrogen
helium
|
|
gptkbp:formed
|
primordial gas
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Population III stars
|
|
gptkbp:is_associated_with
|
the first galaxies
|
|
gptkbp:is_believed_to
|
existed in the early universe
created heavy elements
|
|
gptkbp:is_characterized_by
|
low metallicity
|
|
gptkbp:is_considered_to_be
|
the first generation of stars
|
|
gptkbp:is_followed_by
|
gptkb:Population_I_stars
|
|
gptkbp:is_said_to_be
|
massive stars
|
|
gptkbp:is_studied_in
|
gptkb:cosmology
|
|
gptkbp:may_have_contributed_to
|
the chemical enrichment of the universe
|
|
gptkbp:may_have_led_to
|
formation of black holes
|
|
gptkbp:preceded_by
|
gptkb:Population_II_stars
|
|
gptkbp:responsible_for
|
reionization of the universe
|
|
gptkbp:bfsParent
|
gptkb:Milky_Way
gptkb:Milky_Way_Galaxy
|
|
gptkbp:bfsLayer
|
5
|