Open Access
Fig. 1
[α/Fe] abundance as a function of [Fe/H] for stars with d < 50 kpc simulated with the BGM. Thin and thick disks as well as bulge and halo stars are represented by red, blue, green, and yellow dots, respectively. Black lines indicate the selected population we used here: −2.14 < [Fe/H] < 0.51 and 0 < [α/Fe] < 0.3.
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