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Blinnikov, S.I.; Imshennik, V.S.; Utrobin, V.P.
Gosudarstvennyj Komitet po Ispol'zovaniyu Atomnoj Ehnergii SSSR, Moscow. Inst. Teoreticheskoj i Ehksperimental'noj Fiziki1982
Gosudarstvennyj Komitet po Ispol'zovaniyu Atomnoj Ehnergii SSSR, Moscow. Inst. Teoreticheskoj i Ehksperimental'noj Fiziki1982
AbstractAbstract
[en] The analytic solution of equations for the evolution of supernova remnants in the radiative phase is found. It shows that the X-ray source Cygnus Superbubble might be formed by an explosion with the energy release 1052-1053 erg. The analysis of the light curve of SN 1961 shows that this supernova in the result of an explosion with energy about 2x1052 erg in a supermassive star with the mass of order 103M * where M* is the solar mass. An evolutionary sequence for the formation of giant shell sources is suggested: presupernova - an object of the type R136a, supernova - an explosion of the type SN 1961 and the supernova remnant - a source of the type Cygnus Superbubble
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1982; 20 p; 36 refs.; 1 fig.
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