Statements (55)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:Supernova
|
gptkbp:are |
one of the most energetic events in the universe
|
gptkbp:are_a_key_source_of |
gptkb:Nexon
|
gptkbp:are_a_significant_source_of |
cosmic rays
|
gptkbp:are_often_studied_using |
gptkb:spectroscopy
|
gptkbp:are_part_of |
life cycle of massive stars
|
gptkbp:can_create |
pulsars
|
gptkbp:can_detect |
space telescopes
radio telescopes ground-based telescopes |
gptkbp:can_lead_to |
the formation of supernova remnants
the ejection of stellar material into space |
gptkbp:characterized_by |
core-collapse
|
gptkbp:emissions_standard |
hydrogen lines in their spectra
|
gptkbp:has_a_focus_on |
observational campaigns in astronomy.
|
gptkbp:have_a_typical_peak_brightness_of |
around -17 to -19 magnitudes
|
https://www.w3.org/2000/01/rdf-schema#label |
Type II supernovae
|
gptkbp:is_a_source_of |
gptkb:gravitational_waves
iron in the universe |
gptkbp:is_analyzed_in |
cosmological distances
|
gptkbp:is_associated_with |
gamma-ray bursts in some cases
|
gptkbp:is_essential_for |
the lifecycle of galaxies
cosmic chemical evolution the fate of massive stars the synthesis of elements in the universe |
gptkbp:is_linked_to |
the production of heavy elements like gold and silver
the formation of neutron star mergers |
gptkbp:is_observed_in |
gptkb:the_Milky_Way_galaxy
infrared wavelengths various galaxies different wavelengths of light ultraviolet wavelengths nearby galaxies |
gptkbp:is_often_accompanied_by |
a supernova remnant phase
|
gptkbp:is_often_associated_with |
H II regions
the death of red supergiant stars the formation of planetary nebulae after the explosion |
gptkbp:is_studied_for |
stellar evolution
the expansion of the universe |
gptkbp:is_studied_in |
astrophysics
stellar nucleosynthesis |
gptkbp:is_targeted_at |
mergers of binary stars in some scenarios
|
gptkbp:is_tested_for |
theories of stellar evolution
|
gptkbp:occurs_in |
star-forming regions
massive stars greater than 8 solar masses |
gptkbp:produces |
gptkb:Supernova
black holes |
gptkbp:released |
heavy elements into the interstellar medium
|
gptkbp:research_areas |
modern astrophysics
|
gptkbp:result |
massive star exhaustion of nuclear fuel
|
gptkbp:scientific_classification |
different subtypes based on light curves
Type II-P and Type II-L based on light curve behavior |
gptkbp:trigger_type |
star formation in surrounding gas clouds
|
gptkbp:bfsParent |
gptkb:Wolf
|
gptkbp:bfsLayer |
4
|