Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..374....3w&link_type=abstract
From Stars to Galaxies: Building the Pieces to Build Up the Universe. ASP Conference Series, Vol. 374, proceedings of the confer
Physics
Scientific paper
Primordial stars can be understood as either the very first stars in the Universe, originating from truely primordial, zero-metallicity matter, or as those stars in a (our) galaxy still present with the lowest amounts of metals. I first review aspects of the formation and evolution of the zero-metal stars and then turn to the ultra metal-poor stars in the Galaxy. Many of them have unusual abundances of light, s-process and/or r-process elements. Understanding their origin, in connection with the nucleosynthesis in both the zero-metal and the ultra metal-poor stars, allows to unveil the properties of the very first population of stars and the earliest phase of the galacto-chemical evolution.
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