Supernova models with slow energy pumping and galactic supernova remnants |
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Authors: | V. P. Utrobin |
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Affiliation: | (1) Institute of Applied Mathematics, U.S.S.R. Academy of Sciences, Moscow, USSR |
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Abstract: | The study of supernova (SN) models with slow energy pumping is continued. At maximum luminosity the main characteristics of a SN are shown to be independent of the initial structure of the model (Table I, Figure 1). However, they depend on the massMe of the envelope, and on the intensity of energy pumpingL, with an increase ofMe leading qualitatively to the same changes in the SN parameters as a decrease inL (Table I, Figures 2 and 3). A simple relationship connecting the important SN parameters is obtained (Equation (6)). From the inflection of the color indexB-V curve, the possibility of deriving the characteristic time of energy pumping with intensityL 1044 erg s–1 is pointed out. The comparison of the extragalactic type I SN observations with the results of calculations leads to the estimate ofMe 0.3–0.7M.An investigation of the galactic type I SN remnants is carried out (Table III). The estimate ofMe 0.2–0.3M is obtained for the remnants of supernovae SN 1006, SN 1572, and SN 1604. It completely fits the results for the extragalactic type I SNs. The total initial mass of SN 1604 presupernova was shown to be at least about 7M.It was established that the Crab nebula resulted from the outburst of a peculiar SN. The unique properties of such SNs, including SN 1054, are due to the low intensity of energy pumping (L 1042 erg s–1). The mass of the envelope of the Crab nebula is evaluated to beMe 0.7M. SN 1054 was shown to have mmaxv=–4m.0 at maximum luminosity. |
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