Supernova Remnants

GPTKB entity

Properties (55)
Predicate Object
gptkbp:instanceOf astronomical object
gptkbp:almaMater impact on galaxy evolution
gptkbp:area stellar winds
massive stars
gptkbp:canBe observed in various wavelengths
gptkbp:canEstablish complex structures
varied morphologies
gptkbp:canLeadTo new star formation
gptkbp:composedOf ejected material
gptkbp:contains neutron stars
pulsars
gptkbp:diedIn galactic chemical evolution
gptkbp:exhibitedAt radiation
gptkbp:formed supernova explosion
gptkbp:hasInfluenceOn galactic dynamics
https://www.w3.org/2000/01/rdf-schema#label Supernova Remnants
gptkbp:includes gptkb:SN_1987A
gptkb:Tycho's_Supernova
Cassiopeia A
Crab Nebula
gptkbp:isCharacterizedBy expanding shells
shock_waves
gptkbp:isCitedIn multi-wavelength astronomy
gptkbp:isCounteredBy stellar populations
gptkbp:isFoundIn galaxies
star-forming regions
gptkbp:isImportantFor cosmology
the universe's expansion
understanding stellar evolution
gptkbp:isIncorporatedIn H-alpha emission
gptkbp:isLocatedIn interstellar medium
gptkbp:isOftenMadeWith cosmic rays
gamma-ray bursts
gptkbp:isPartOf supernova remnants catalogues
gptkbp:isStudiedIn astrophysics
computer simulations
their magnetic fields
their particle acceleration
gptkbp:isSuitableFor dark energy theories
gptkbp:isUsedBy the origins of elements.
gptkbp:isUsedFor radio telescopes
X-ray telescopes
different galaxies
their age
optical telescopes
test theories of gravity
Type II remnants
shock wave theory
interstellar_medium_dynamics
Type_Ia_remnants
gptkbp:isUtilizedFor the nature of black holes
gptkbp:keyIssues understanding dark matter
the life cycle of stars
gptkbp:mayHave chemical composition
insight into nucleosynthesis