Type II-P supernovae

GPTKB entity

Statements (53)
Predicate Object
gptkbp:instance_of gptkb:nebula
gptkbp:bfsLayer 5
gptkbp:bfsParent gptkb:SN_1979_C
gptkbp:affects surrounding interstellar medium
gptkbp:apparent_magnitude -17.5 to -18.5
gptkbp:are type of core-collapse supernova
gptkbp:associated_with massive stars
gptkbp:can_create gptkb:physicist
black holes
gptkbp:can_lead_to the formation of neutron star mergers
gptkbp:common_name their light curve characteristics
gptkbp:exhibits hydrogen lines
gptkbp:focuses_on observational astronomy
gptkbp:has_exit gptkb:supernova_remnants
gptkbp:have luminosity decline
https://www.w3.org/2000/01/rdf-schema#label Type II-P supernovae
gptkbp:is_a_source_of heavy elements
gptkbp:is_aimed_at stellar evolution
gptkbp:is_analyzed_in cosmological distances
light curve behavior
stellar nucleosynthesis processes
gptkbp:is_associated_with gamma-ray bursts
Type IIP supernovae.
gptkbp:is_characterized_by plateau phase
gptkbp:is_essential_for the universe's expansion
nucleosynthesis
gptkbp:is_explored_in gptkb:Monarch
gptkbp:is_featured_in astronomical surveys
gptkbp:is_found_in star-forming regions
gptkbp:is_influenced_by environmental factors
gptkbp:is_linked_to gptkb:Wolf-Rayet_stars
stellar population studies
gptkbp:is_observed_in in various wavelengths
in nearby galaxies
in the infrared spectrum
gptkbp:is_often_compared_to Type II-L supernovae
gptkbp:is_part_of stellar lifecycle
the supernova classification scheme
gptkbp:is_studied_in in astrophysics
their explosion mechanisms
gptkbp:is_tested_for supernova models
gptkbp:occurs_in galaxies
isolated stars
gptkbp:provides_information_on cosmological simulations
stellar masses
gptkbp:recognizes by ground-based telescopes
by space telescopes
gptkbp:research cosmic evolution
gptkbp:research_areas astrophysics
gptkbp:result core collapse
gptkbp:scientific_classification gptkb:Type_II_supernovae
gptkbp:significance galactic chemical evolution
the study of supernova remnants