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The 46 pages that link to Supernova remnant, each with the reason it gives.

• Interstellar mediumBroader topic: Supernovae heat, compress, and enrich the medium, driving much of its turbulence.

• X-ray astronomyRelated: X-rays map hot shock-heated gas and the elements forged in stellar explosions.

• SupernovaBroader topic: It is the evolving debris produced by the explosion.

• Shock waveRelated: Its outward shock wave heats and compresses interstellar gas.

• Cosmic rayRelated: Shock acceleration in remnants is a leading explanation for many Galactic cosmic rays.

• Core-collapse supernovaNarrower topic: It records the explosion’s interaction with surrounding material over thousands of years.

• Gamma-ray astronomyRelated: Gamma rays from remnants can reveal interactions between accelerated particles and surrounding matter or radiation.

• Supernova nucleosynthesisBroader topic: Remnant spectra and composition provide observational evidence of synthesized ejecta.

• SN 1987ANarrower topic: SN 1987A is evolving into a remnant as its ejecta strike the inner ring.

• Crab NebulaNarrower topic: The Crab’s nebula is the observable remnant of the 1054 explosion.

• Emission nebulaCompared with: Some remnants emit nebular lines, but shock heating rather than nearby stellar ultraviolet often powers their glow.

• Herbig–Haro objectCompared with: Both involve shock emission, but a supernova remnant is powered by an exploded star.

• Population III starRelated: First-star remnants dispersed newly forged elements and influenced nearby gas collapse.

• NebulaBroader topic: Some nebulae are shaped by shock waves and ejecta from supernovae.

• Red supergiantRelated: A red-supergiant explosion can leave a remnant enriched by its outer layers.

• Rayleigh–Taylor instabilityBroader topic: Rayleigh–Taylor mixing helps distribute stellar ejecta through the remnant.

• Cassiopeia ANarrower topic: Cassiopeia A is a nearby, young example of this class of object.

• Interstellar magnetic fieldRelated: Supernova shocks can compress and amplify magnetic fields in the surrounding interstellar medium.

• Pulsar wind nebulaRelated: Many pulsar wind nebulae expand within the debris of the supernova that formed their pulsar.

• Eta CarinaeCompared with: Eta Carinae’s nebula formed before any confirmed terminal explosion, unlike a supernova remnant.

• Tarantula NebulaRelated: Past supernovae have added shock waves and energy to the nebula's complex environment.

• Crab PulsarNarrower topic: The Crab Pulsar showed that a compact remnant can actively power a supernova remnant.

• Einstein ObservatoryRelated: Einstein resolved X-ray emission from remnants, revealing hot structures within the debris.

• X-ray telescopeRelated: X-ray observations map shock-heated gas and compact objects within these expanding remnants.

• Fermi Gamma-ray Space TelescopeRelated: Fermi observations test whether these remnants accelerate cosmic rays that produce gamma rays.

• Reflection nebulaCompared with: Its glow is powered chiefly by shocked or energized gas rather than reflected starlight.

• XMM-NewtonRelated: XMM-Newton detects the hot plasma and energetic processes in these remnants.

• Astrophysical fluid dynamicsBroader topic: Their evolution is governed by blast-wave fluid dynamics and interactions with ambient gas.

• Astrophysical maserRelated: Some masers arise where supernova-driven shocks compress and excite molecular gas.

• Superluminous supernovaNarrower topic: The late-time debris can preserve evidence about the explosion's energy source.

• Kepler's SupernovaNarrower topic: The visible nebula is the surviving debris of the 1604 explosion.

• Messier 82Related: Overlapping explosions help energize M82’s outflow and its bright radio emission.

• SN 1054Narrower topic: The Crab Nebula is the evolving remnant of the explosion.

• Galactic astronomyRelated: Remnants reveal how stellar deaths inject energy and elements into the interstellar medium.

• High-energy astrophysicsBroader topic: Its shocks can accelerate cosmic rays and emit X-rays and gamma rays.

• Interstellar cloudRelated: Its shock waves can compress interstellar clouds and trigger or disrupt collapse.

• NGC 6302Compared with: Unlike this explosion-driven structure, NGC 6302 formed from material shed by a star without a supernova.

• NGC 6946Narrower topic: The remnants preserve evidence of earlier explosions between recorded supernova events.

• ROSATRelated: ROSAT surveys mapped remnants and traced hot gas from supernova explosions.

• SN 1572Narrower topic: The event’s surviving debris can be studied long after its light faded.

• Astronomical radio sourceBroader topic: Its magnetized, energetic particles produce extended synchrotron radio emission.

• Astrophysical X-ray sourceBroader topic: Shock-heated ejecta and swept-up gas glow in X-rays.

• Cosmic rays and astroparticlesRelated: Its shocks are candidate sources of Galactic cosmic rays.

• Cygnus LoopNarrower topic: The Cygnus Loop is a nearby, extended example of this class of object.

• Laboratory studies of space and astrophysical plasmasBroader topic: Scaled experiments investigate shock formation and magnetic-field growth in remnants.

• Stochastic self-propagating star formation modelBroader topic: An expanding remnant can sweep up gas into a shell where stars may form.