Abstract
Most of the work reported here has been conducted within the ESO Large Programme 165.N-0276 “Galaxy Formation, Early Nucleosynthesis, and the First Stars”, which has covered 4 periods 65–68, from April 2000 to November 2001, with a total of 38 nights in visitor mode. The team had R. Cayrel as PI, and 13 CoIs:
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Cayrel, R., Spite, M. (2006). First Stars: Abundance Patterns from O to Zn and Derived SNe Yields in the Early Galaxy. In: Randich, S., Pasquini, L. (eds) Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-34136-9_41
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DOI: https://doi.org/10.1007/978-3-540-34136-9_41
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