Statements (55)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:nebula
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:core-collapse_supernovae
|
| gptkbp:associated_with |
gptkb:Wolf-Rayet_stars
gamma-ray bursts Type I Ib supernovae mass loss in progenitor stars |
| gptkbp:bomb_load |
around 1-2 x 10^51 ergs
|
| gptkbp:can_lead_to |
formation of neutron stars or black holes
|
| gptkbp:conservation_efforts |
can form supernova remnants
|
| gptkbp:contribution |
stellar nucleosynthesis
chemical enrichment of the universe understanding of supernova rates |
| gptkbp:creator |
massive stars
|
| gptkbp:discovered_by |
gptkb:observatory
|
| gptkbp:distance |
can be observed at great distances
|
| gptkbp:example |
gptkb:SN_2016gkg
gptkb:SN_1999ex gptkb:SN_2008_D gptkb:SN_2012au gptkb:SN_2013df |
| gptkbp:first_appearance |
gptkb:1987_A
|
| gptkbp:frequency |
less frequent than Type II supernovae
|
| gptkbp:has_spectral_type |
absence of hydrogen lines
|
| gptkbp:hosts |
spiral galaxies
|
| https://www.w3.org/2000/01/rdf-schema#label |
Type Ib supernovae
|
| gptkbp:impact |
chemical evolution of galaxies
understanding of galaxy formation cosmology research |
| gptkbp:influence |
galactic evolution
stellar population studies |
| gptkbp:is_characterized_by |
helium-rich spectra
|
| gptkbp:is_observed_in |
gptkb:Chandra_X-ray_Observatory
gptkb:Hubble_Space_Telescope various wavelengths ground-based telescopes |
| gptkbp:lighting |
can vary significantly
plateau phase can exhibit diverse behaviors can reach up to -17.3 magnitude declines more slowly than Type II supernovae provides insights into progenitor properties used to estimate distances |
| gptkbp:occurs_in |
galaxies
|
| gptkbp:power_output |
significant energy output
|
| gptkbp:related_model |
used to study supernova mechanisms
|
| gptkbp:related_to |
gptkb:Type_Ic_supernovae
|
| gptkbp:research |
gptkb:musician
difficult to observe in distant galaxies help understand stellar evolution used to refine cosmological models |
| gptkbp:research_focus |
important for understanding dark energy
|
| gptkbp:result |
core collapse of a massive star
|
| gptkbp:theory |
focus on explosion mechanisms
|
| gptkbp:type |
core-collapse supernova
|