The Element Abundances in Meta-l poor Stars and Nucleosynthetic Yield of SNe ???
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Abstract
Adopting the same method as Tsujimoto used, this paper calculates the A-element and Fe-group element yields of SNe ??? with various masses from the latest observed element abundance and the theoretical yield of Si given by WW95 and FM2004. The previous results and results obtained in this paper are also compared.
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