Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing
We present results of a detailed chemical analysis performed on 23 main-sequence turnoff stars having -3.4 ≤ [Fe/H] ≤ -2.2, a sample selected to be highly homogeneous in Teff and log(g). We investigate the efficiency of mixing in the early Galaxy by m
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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