Nucleosynthesis in Metal-Free and Metal-Poor Stars

Details Nucleosynthesis in Metal-Free and Metal-Poor Stars Nucleosynthesis in Metal-Free and Metal-Poor Stars

2008-07-04

arxiv.org/abs/0807.0818v1

Astronomy and Astrophysics

Astrophysics

8 pages, no figures, published in "Proceedings of First Stars III," Eds. Brian W. O'Shea, Alexander Heger & Tom Abel

Scientific paper

10.1063/1.2905564

There have been a number of important recent developments in theoretical and observational studies of nucleosynthesis, especially regarding nucleosynthetic sources at low metallicities. Those selected for discussion here include the origin of Li6, the primary production of N, the s-process, and the supernova sources for three groups of metals: (1) C to Zn with mass numbers A<70, (2) Sr to Ag with A~90-110, and (3) r-process nuclei with A~130 and above.

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