Fig. 6
[Mg/Fe] vs. [Fe/H] and [O/Mg] vs. [Fe/H] data from the literature for thick disk and bulge stars are compared to the predictions of the model with a specific star-formation rate of νSF = 3 Gyr-1. The references for the data points are: Alves-Brito et al. (2010), Hill et al. (2011), Bensby et al. (2013), Johnson et al. (2014), Gonzalez et al. (2015) and Ryde et al. (2016).
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