Statements (50)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:affects |
stellar populations
|
| gptkbp:are_part_of |
stellar evolution
|
| gptkbp:are_typically_found_in |
gptkb:the_Milky_Way
|
| gptkbp:can_be_used_to |
study cosmic rays
study stellar nucleosynthesis study supernova explosions |
| gptkbp:can_be_used_to_examine |
galactic magnetic fields
|
| gptkbp:can_contain |
gptkb:Supernova
black holes |
| gptkbp:can_create |
shock waves
|
| gptkbp:can_detect |
gamma-ray telescopes
|
| gptkbp:can_lead_to |
star formation
|
| gptkbp:eject |
heavy elements
|
| gptkbp:exhibits |
thermal emission
non-thermal emission |
| gptkbp:expand_at |
high velocities
|
| https://www.w3.org/2000/01/rdf-schema#label |
Type II supernova remnants
|
| gptkbp:influence |
galactic dynamics
|
| gptkbp:is_analyzed_in |
gptkb:interstellar_medium
astrophysics research cosmic microwave background cosmic dust stellar mass loss |
| gptkbp:is_associated_with |
gptkb:Wolf-Rayet_stars
massive stars red supergiants |
| gptkbp:is_characterized_by |
hydrogen-rich spectra
|
| gptkbp:is_described_as |
supernova rates
|
| gptkbp:is_essential_for |
cosmic chemical evolution
|
| gptkbp:is_explored_in |
galactic evolution
|
| gptkbp:is_found_in |
galaxies
|
| gptkbp:is_often_compared_to |
gptkb:Type_Ia_supernova_remnants
asymmetric observed in infrared |
| gptkbp:is_often_seen_in |
star-forming regions
|
| gptkbp:is_recognized_by |
light curves
|
| gptkbp:is_related_to |
Type I supernova remnants
|
| gptkbp:is_studied_for |
elemental abundances
their impact on surrounding gas |
| gptkbp:is_studied_in |
gptkb:spectroscopy
X-ray astronomy radio astronomy optical astronomy |
| gptkbp:key |
understanding supernova mechanics
|
| gptkbp:result |
core-collapse supernova
|
| gptkbp:scientific_classification |
plasma remnants
shell-type remnants |
| gptkbp:bfsParent |
gptkb:Type_Ia_supernova_remnants
|
| gptkbp:bfsLayer |
7
|