Statements (74)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:bfsLayer |
3
|
| gptkbp:bfsParent |
gptkb:Milky_Way
gptkb:Milky_Way_Galaxy |
| gptkbp:age |
younger than 10 billion years
|
| gptkbp:are |
often studied in astrophysics
often found in regions of active star formation often studied in relation to cosmic microwave background radiation often studied in relation to dark matter important for understanding galaxy evolution often used in the study of the universe's expansion often found in the vicinity of other Population I stars often found in the vicinity of active galactic nuclei associated with the formation of planetary systems often studied in relation to stellar nucleosynthesis more chemically diverse than Population II stars more luminous than Population II stars often associated with the interstellar medium often found in regions of high star density often found in the vicinity of blue supergiants often found in the vicinity of gamma-ray bursts often found in the vicinity of nebulae often found in the vicinity of quasars often found in the vicinity of red giants often found in the vicinity of supernova remnants often involved in supernova events often involved in the formation of black holes often involved in the formation of carbon stars often involved in the formation of galaxies often involved in the formation of neutron stars often involved in the formation of new stars often involved in the formation of star clusters often involved in the formation of supergiants often involved in the formation of white dwarfs often part of the galactic bulge often part of the galactic disk often part of the galactic halo often studied in relation to cosmic rays often studied in relation to gravitational waves often studied in relation to stellar evolution often studied in relation to the cosmic web often used in the search for exoplanets often used in the study of galactic dynamics often used in the study of stellar populations younger than Population II stars younger than Population III stars important for the chemical enrichment of the universe often studied in relation to the lifecycle of stars often studied in relation to the formation of the solar system often studied in relation to the evolution of the universe often used as standard candles in distance measurement often involved in the recycling of stellar material |
| gptkbp:associated_with |
star-forming regions
open clusters |
| gptkbp:can_be |
be classified by their spectral types
be found in globular clusters exhibit variability form binary systems |
| gptkbp:example |
gptkb:the_Sun
|
| gptkbp:form |
interstellar gas and dust
|
| gptkbp:have |
higher abundance of elements heavier than helium
|
| https://www.w3.org/2000/01/rdf-schema#label |
Population I stars
|
| gptkbp:includes |
O-type stars
B-type stars M-type stars A-type stars G-type stars K-type stars F-type stars |
| gptkbp:is_characterized_by |
high metallicity
|
| gptkbp:is_found_in |
gptkb:the_Milky_Way_galaxy
|
| gptkbp:is_often_associated_with |
planets
|
| gptkbp:located_in |
the spiral arms of galaxies
|
| gptkbp:type |
main sequence stars
|