Statements (52)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:are_key_sources_of |
energy in the universe
|
| gptkbp:are_less_common_than |
smaller stars
|
| gptkbp:are_often_the_first_to |
die in a galaxy.
|
| gptkbp:are_part_of |
the life cycle of matter in the universe
|
| gptkbp:born_in |
massive molecular clouds
|
| gptkbp:can |
high metallicity
multiple stellar companions |
| gptkbp:can_be_found_in |
galactic halos
|
| gptkbp:can_create |
gptkb:stellar_black_holes
gamma-ray bursts |
| gptkbp:can_detect |
their X-ray emissions
|
| gptkbp:contribution |
stellar feedback
|
| gptkbp:created |
gptkb:Supernova
|
| gptkbp:emit_radiation |
in ultraviolet spectrum
|
| gptkbp:exhibits |
pulsations
stellar flares mass loss during their lifetime |
| gptkbp:form_black_holes |
after supernova explosion
|
| gptkbp:has_luminosity |
compared to smaller stars
|
| gptkbp:have_high_rotational_velocities |
compared to smaller stars
|
| gptkbp:have_high_surface_temperatures |
over 30,000 K
|
| gptkbp:have_short_lifespans |
millions of years
|
| gptkbp:have_strong_winds |
due to high temperatures
|
| https://www.w3.org/2000/01/rdf-schema#label |
Massive Stars
|
| gptkbp:influence |
galactic evolution
the formation of new stars |
| gptkbp:is_a_source_of |
cosmic rays
|
| 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
|
| 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
|
| gptkbp:is_often_seen_in |
regions of active star formation
the spiral arms of galaxies |
| gptkbp:is_part_of |
binary systems
|
| gptkbp:is_studied_in |
gptkb:spectroscopy
astrophysics computer simulations |
| gptkbp:key |
understanding cosmic evolution
the lifecycle of galaxies |
| gptkbp:life_cycle |
gptkb:Supernova
|
| gptkbp:mass |
greater than 8 solar masses
|
| gptkbp:produce_heavy_elements |
through nucleosynthesis
|
| gptkbp:scientific_classification |
O-type stars
B-type stars |
| gptkbp:undergo_nuclear_fusion |
hydrogen into helium
|
| gptkbp:bfsParent |
gptkb:Compact_Binary_System
gptkb:Two_Neutron_Stars |
| gptkbp:bfsLayer |
6
|