Statements (52)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:star
|
gptkbp:bfsLayer |
4
|
gptkbp:bfsParent |
gptkb:Compact_Binary_System
gptkb:Two_Neutron_Stars |
gptkbp:beam |
in ultraviolet spectrum
|
gptkbp:born |
massive molecular clouds
|
gptkbp:can_be |
high metallicity
multiple stellar companions |
gptkbp:can_create |
gptkb:stellar_black_holes
gamma-ray bursts |
gptkbp:climate |
over 30,000 K
|
gptkbp:contribution |
stellar feedback
|
gptkbp:created |
gptkb:physicist
|
gptkbp:end_of_life |
gptkb:nebula
|
gptkbp:exhibits |
pulsations
stellar flares mass loss during their lifetime |
gptkbp:formed |
after supernova explosion
|
gptkbp:has_luminosity |
compared to smaller stars
|
https://www.w3.org/2000/01/rdf-schema#label |
Massive Stars
|
gptkbp:influence |
galactic evolution
the formation of new stars |
gptkbp:is_a_fusion_of |
hydrogen into helium
|
gptkbp:is_a_source_of |
cosmic rays
energy in the universe |
gptkbp:is_critical_for |
understanding stellar evolution
|
gptkbp:is_essential_for |
chemical enrichment of the universe
the study of supernova remnants |
gptkbp:is_found_in |
star clusters
galactic halos |
gptkbp:is_observed_in |
nebulae
|
gptkbp:is_often_associated_with |
massive star-forming regions
|
gptkbp:is_often_compared_to |
blue or blue-white in color
die in a galaxy. smaller stars |
gptkbp:is_often_depicted_as |
regions of active star formation
the spiral arms of galaxies |
gptkbp:is_part_of |
binary systems
the life cycle of matter in the universe |
gptkbp:is_studied_in |
gptkb:musician
astrophysics computer simulations |
gptkbp:isotopes |
through nucleosynthesis
|
gptkbp:key |
understanding cosmic evolution
the lifecycle of galaxies |
gptkbp:lifespan |
millions of years
|
gptkbp:mass |
greater than 8 solar masses
|
gptkbp:max_speed |
compared to smaller stars
|
gptkbp:recognizes |
their X-ray emissions
|
gptkbp:scientific_classification |
O-type stars
B-type stars |
gptkbp:weather_conditions |
due to high temperatures
|