Statements (58)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:observatory
|
| gptkbp:bfsLayer |
2
|
| gptkbp:bfsParent |
gptkb:physicist
|
| gptkbp:can_be |
complex structures
multiple components |
| gptkbp:contains |
ejecta
|
| gptkbp:emissions_standard |
gamma rays
|
| gptkbp:example |
stellar evolution
|
| gptkbp:exhibits |
shock waves
synchrotron radiation thermal X-ray emission |
| gptkbp:form |
supernova explosion
|
| gptkbp:has_expansion |
into the interstellar medium
|
| https://www.w3.org/2000/01/rdf-schema#label |
supernova remnants
|
| gptkbp:influence |
galactic dynamics
|
| gptkbp:interacts_with |
molecular clouds
|
| gptkbp:is_analyzed_in |
dark matter interactions
distance to galaxies |
| gptkbp:is_associated_with |
gptkb:physicist
black holes cosmic dust massive stars |
| gptkbp:is_described_as |
galactic evolution
|
| gptkbp:is_essential_for |
chemical enrichment of the galaxy
|
| gptkbp:is_found_in |
gptkb:the_Milky_Way
star clusters other galaxies |
| gptkbp:is_influenced_by |
supernova feedback
|
| gptkbp:is_observed_in |
optical wavelengths
X-ray wavelengths radio wavelengths infrared wavelengths |
| gptkbp:is_often_associated_with |
gptkb:Type_Ia_supernovae
gptkb:Type_II_supernovae |
| gptkbp:is_often_depicted_as |
star-forming regions
the outskirts of galaxies |
| gptkbp:is_part_of |
galactic winds
superbubbles |
| gptkbp:is_studied_in |
gptkb:musician
astrophysics imaging techniques cosmic rays the interstellar medium the life cycle of stars the expansion of the universe their magnetic fields the history of star formation |
| gptkbp:map |
3 D space
|
| gptkbp:monitors |
thermal emission
non-thermal emission |
| gptkbp:named_after |
the constellation they are found in
|
| gptkbp:ray_tracing_support |
stellar populations
|
| gptkbp:recognizes |
space telescopes
ground-based telescopes |
| gptkbp:scientific_classification |
pulsar wind nebulae
plasma remnants shell-type remnants |
| gptkbp:trigger_type |
star formation
|