Carbon-rich, extremely metal-poor Population II stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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4 pages including 1 figure. Conference proceedings for "CNO in the Universe", St Luc, Switzerland, 10-14 September 2002 C. Cha

Scientific paper

A significant fraction of very metal-poor stars have unexpectedly high carbon
abundances. I recap on their discovery, describe the results of high-resolution
spectroscopic studies of their composition, and consider possible origins. It
is now clear that at least two, and possibly three different explanations are
needed for their general characteristics.

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