The Element Abundances in Metal-Poor Stars and Nucleosynthesis Yield of SNe II

Details The Element Abundances in Metal-Poor Stars and Nucleosynthesis Yield of SNe II The Element Abundances in Metal-Poor Stars and Nucleosynthesis Yield of SNe II

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007pnaoc...4...95m&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 4, No.

Astronomy and Astrophysics

Astronomy

Extremely Metal-Poor Stars, Element Abundances, Supernovae Ii, Nucleosynthesis

Scientific paper

Adopting the same method as Tsujimoto used, this paper calculates the α-element and Fe-group element yields of SNe II with various masses from the latest observed element abundance and the theoretical yield of Si given by WW95 (Woosley and Weaver, 1995) and FM2004 (François, Mateucci et al., 2004). The previous results and results obtained in this paper are also compared.

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