The Evolution of the C/O Ratio in Metal-poor Halo Stars
We report new measurements of carbon and oxygen abundances in 34 F and G dwarf and subgiant stars belonging to the halo population and spanning a range of metallicity from [Fe/H] = -0.7 to -3.2. The survey is based on observations of four permitted lines
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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