Statements (64)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:astronomy
|
| gptkbp:are_often_cataloged_in |
astronomical surveys
|
| gptkbp:are_remnants_of |
massive stars
|
| gptkbp:can |
complex structures
|
| gptkbp:can_be_found_in |
galaxies
|
| gptkbp:can_be_studied_to_learn_about |
the early universe
stellar nucleosynthesis |
| gptkbp:can_be_studied_to_understand |
the dynamics of the universe
the expansion of the universe the fate of massive stars |
| gptkbp:can_contain |
gptkb:Supernova
molecular clouds black holes |
| gptkbp:can_create |
cosmic rays
|
| gptkbp:can_detect |
infrared observations
|
| gptkbp:emissions_standard |
gptkb:X-rays
radio waves optical light |
| gptkbp:exhibits |
thermal emission
|
| gptkbp:expansion |
over thousands of years
|
| gptkbp:formed |
the explosion of a supernova
|
| https://www.w3.org/2000/01/rdf-schema#label |
Supernova Remnants
|
| gptkbp:influence |
star formation processes
|
| gptkbp:interacts_with |
the surrounding interstellar medium
|
| gptkbp:is_a_site_for |
new star formation
chemical reactions. |
| gptkbp:is_a_source_of |
gptkb:cosmic_ray_detector
light elements heavy elements |
| gptkbp:is_affected_by |
supernova shock waves
|
| gptkbp:is_analyzed_in |
cosmological distances
|
| gptkbp:is_associated_with |
gptkb:Type_Ia_supernovae
gptkb:Type_II_supernovae stellar nurseries cosmic dust stellar explosions the end stages of stellar evolution |
| gptkbp:is_essential_for |
the chemical enrichment of the interstellar medium
|
| gptkbp:is_influenced_by |
magnetic fields
|
| gptkbp:is_linked_to |
gamma-ray bursts
the formation of black holes the formation of neutron stars |
| gptkbp:is_observed_in |
gptkb:the_Milky_Way
various wavelengths infrared wavelengths other galaxies |
| gptkbp:is_often_associated_with |
pulsars
|
| gptkbp:is_often_seen_in |
galactic regions of star formation
|
| gptkbp:is_part_of |
galactic evolution
superbubbles |
| gptkbp:is_studied_for |
the interstellar medium
|
| gptkbp:is_studied_in |
astrophysics
radio telescopes optical telescopes X-ray observatories their role in stellar evolution |
| gptkbp:monitors |
shock waves
|
| gptkbp:provides_information_on |
the life cycle of stars
|
| gptkbp:scientific_classification |
plasma remnants
shell-type remnants mixed-morphology remnants |
| gptkbp:bfsParent |
gptkb:Supernova
gptkb:astronomy |
| gptkbp:bfsLayer |
4
|