the Vela Supernova Remnant

GPTKB entity

Statements (56)
Predicate Object
gptkbp:instance_of gptkb:nebula
gptkbp:age approximately 11,000 years
gptkbp:contains gptkb:pulsar_PSR_B0833-45
heavy elements
gptkbp:depicted_in Southern Hemisphere
southern sky
H-alpha emissions
gptkbp:diameter about 30 light years
gptkbp:discovered_by Australian astronomers
gptkbp:distance about 800 light years
gptkbp:emissions_standard gptkb:X-rays
gptkbp:founded supernova explosion
gptkbp:has_method shell-like structure
gptkbp:has_spectral_type non-thermal spectrum
https://www.w3.org/2000/01/rdf-schema#label the Vela Supernova Remnant
gptkbp:is_associated_with gptkb:interstellar_medium
cosmic rays
gamma-ray emissions
stellar remnants
gptkbp:is_considered_as a prototype for supernova remnants
gptkbp:is_known_for its historical significance
its role in star formation
its interaction with surrounding gas
its pulsar
its bright X-ray emission
its large angular size
gptkbp:is_located_near the Gum Nebula
gptkbp:is_observed_in optical wavelengths
radio wavelengths
infrared wavelengths
gptkbp:is_part_of gptkb:Vela_SNR_complex
gptkb:Milky_Way_galaxy
Galactic Plane
the Local Bubble
the Galactic Center region
the Vela constellation
supernova remnant catalog
the Vela Pulsar System
the Vela constellation's mythology
the interstellar medium's dynamics
gptkbp:is_studied_in astrophysics
magnetic fields
shock waves
stellar evolution
radio telescopes
thermal emissions
optical telescopes
elemental abundances
X-ray observatories
cosmic ray acceleration
neutrino emissions
radiative shocks
gptkbp:lighting high surface brightness
gptkbp:located_in gptkb:Vela_constellation
gptkbp:bfsParent gptkb:Vela
gptkbp:bfsLayer 4