The First Stars: What We Know and Do Not Know

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Scientific paper

The H and K survey of Beers, Preston & Shectman has been the mine of extremely metal-poor stars during the last decade of the XXth century. The VLT-UVES combination has allowed us to study the chemical composition of the brightest members of this population, fossil component of events which have occured either during the formation of the galaxy, or earlier in smaller systems having eventually merged into our beautiful milky way. We report here what has been derived from a VLT large programme devoted to these objects, as well as on other questions relevant to the first stars.

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