Fig. 2.
[Mg/Fe], [Mn/Fe], [Ni/Fe], and [Zn/Fe] as a function of [Fe/H] for stars in Nissen & Schuster (2010, 2011). Stars belonging to the high-α sequence are shown with blue circles and those on the low-α sequence with filled red circles. The components of G 112-43/44 are indicated with a black square. Typical 1σ errors of the differential abundance ratios are shown at the bottom of each panel.
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