Cygnus Superbubble as the remnant of a peculiar supernova
Sergei I. Blinnikov, В. С. Имшенник, В. П. Утробин
Abstract
Sergei I. Blinnikov, В. С. Имшенник, В. П. Утробин
Abstract
An analytic solution is obtained for the evolution of a supernova remnant during the radiative-cooling phase. The Cygnus Superbubble x-ray source could have been formed by the explosion of a single supernova releasing an energy of 10/sup 52/--10/sup 53/ erg. Analysis of the light curve of the NGC 1058 supernova 1961v demonstrates that it represents a roughly-equal2 x 10/sup 52/ erg outburst of a supermassive (roughly-equal10/sup 3/ M/sub sun/) star. Giant shell sources may form an evolutionary sequence, exemplified by R136a as the presupernova, supernova 1961v, and the Superbubble as the remnant.
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An analytic solution is obtained for the evolution of a supernova remnant during the radiative-cooling phase. The Cygnus Superbubble x-ray source could have been formed by the explosion of a single supernova releasing an energy of 10/sup 52/--10/sup 53/ erg. Analysis of the light curve of the NGC 1058 supernova 1961v demonstrates that it represents a roughly-equal2 x 10/sup 52/ erg outburst of a supermassive (roughly-equal10/sup 3/ M/sub sun/) star. Giant shell sources may form an evolutionary sequence, exemplified by R136a as the presupernova, supernova 1961v, and the Superbubble as the remnant.
Key concepts: Superbubble, Supernova, Physics, Astrophysics, Supernova remnant, Astronomy, Erg, Type II supernova