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G299 Type Ia supernova remnant.
G299 Type Ia supernova remnant.
An accretion disc forms around a compact body (such as a white dwarf) stripping gas from a companion giant star. NASA image
An accretion disc forms around a compact body (such as a white dwarf) stripping gas from a companion giant star. NASA image
Supercomputer simulation of the explosion phase of the deflagration-to-detonation model of supernova formation.
Supercomputer simulation of the explosion phase of the deflagration-to-detonation model of supernova formation.
Supernova remnant N103B taken by the Hubble Space Telescope.
Supernova remnant N103B taken by the Hubble Space Telescope.
SN 1994D (bright spot on the lower left), a Type Ia supernova within its host galaxy, NGC 4526
SN 1994D (bright spot on the lower left), a Type Ia supernova within its host galaxy, NGC 4526
The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova.
The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova.
A 1414 text cites a 1055 report: since "the baleful star appeared, a full year has passed and until now its brilliance has not faded".
A 1414 text cites a 1055 report: since "the baleful star appeared, a full year has passed and until now its brilliance has not faded".
Supernova remnant SNR E0519-69.0 in the Large Magellanic Cloud
Supernova remnant SNR E0519-69.0 in the Large Magellanic Cloud