Carbon-rich, Extremely Metal-Poor Population II stars

Ryan, Sean G. (2003) Carbon-rich, Extremely Metal-Poor Population II stars. In: UNSPECIFIED.

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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.

Item Type	Conference or Workshop Item (Other)
Additional information	Original paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical Society of the Pacific
Date Deposited	15 May 2025 16:18
Last Modified	10 Jul 2025 23:21