Stellar Population I

GPTKB entity

Statements (64)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:age Stellar Population II
Stellar Population III
gptkbp:age_group less than 10 billion years
gptkbp:characterized_by young stars
gptkbp:composed_of hydrogen and helium
https://www.w3.org/2000/01/rdf-schema#label Stellar Population I
gptkbp:includes blue stars
main sequence stars
open clusters
metal-rich stars
gptkbp:is_associated_with star formation regions
the interstellar medium
massive stars
the Galactic Center
the Milky Way's spiral arms
the Galactic Halo
the Orion Arm
gptkbp:is_characterized_by variable stars
high luminosity
high metallicity
rapid rotation
high star formation rate
gptkbp:is_connected_to gptkb:supernova_remnants
the formation of planetary systems
the cosmic web
gptkbp:is_dominant_in the solar neighborhood
gptkbp:is_essential_for gptkb:cosmology
stellar classification
understanding galaxy evolution
understanding star formation history
gptkbp:is_examined_in gptkb:spectroscopy
photometry
computer simulations
gptkbp:is_found_in gptkb:starburst_galaxies
gptkb:the_Milky_Way_Galaxy
gptkb:the_Local_Group
spiral galaxies
the Local Supercluster
the Galactic Bulge
gptkbp:is_influenced_by gptkb:interstellar_medium
stellar winds
galactic winds
gptkbp:is_involved_in nuclear fusion processes
gptkbp:is_located_in the galactic disk
gptkbp:is_observed_in Hubble Space Telescope images
nearby galaxies
gptkbp:is_part_of the Milky Way's structure
gptkbp:is_related_to stellar evolution
stellar populations
the Hertzsprung-Russell diagram
stellar clusters
the cosmic microwave background
gptkbp:is_studied_for stellar dynamics
galactic chemical evolution
the lifecycle of stars
gptkbp:is_studied_in astrophysics
stellar astrophysics
galactic archaeology
gptkbp:key the formation of the Milky Way
gptkbp:scientific_classification young stellar objects
gptkbp:bfsParent gptkb:The_Sun
gptkb:Sun
gptkbp:bfsLayer 5