The Element Abundances in Meta-l poor Stars and Nucleosynthetic Yield of SNe ???

MA Wen-juan; ZHOU Gui-de; ZHANG Bo

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Astronomical Research and Technology > 2007 > 4(2): 95-101.

MA Wen-juan, ZHOU Gui-de, ZHANG Bo. The Element Abundances in Meta-l poor Stars and Nucleosynthetic Yield of SNe ???[J]. Astronomical Research and Technology, 2007, 4(2): 95-101.

Citation:

MA Wen-juan, ZHOU Gui-de, ZHANG Bo. The Element Abundances in Meta-l poor Stars and Nucleosynthetic Yield of SNe ???[J]. Astronomical Research and Technology, 2007, 4(2): 95-101.

Citation:

MA Wen-juan, ZHOU Gui-de, ZHANG Bo. The Element Abundances in Meta-l poor Stars and Nucleosynthetic Yield of SNe ???[J]. Astronomical Research and Technology, 2007, 4(2): 95-101.

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The Element Abundances in Meta-l poor Stars and Nucleosynthetic Yield of SNe ???

1.
Physics Department, Cangzhou Teachers'College, Hebei Cangzhou 061001, China
2.
College of Physics, Hebei Normal University, Hebei Shijiazhuang 050016, China

More Information

Received Date: July 10, 2006
Revised Date: September 10, 2006
Published Date: April 14, 2007

Graphical Abstract

Abstract

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.
- extremely meta-l poor stars,
- element abundance,
- SNe ???,
- nucleosynthesis