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Fig. 4

image

Difference in non-LTE Mg abundance Δ[Mg/Fe]NLTE versus stellar metallicity for a fixed LTE difference Δ[Mg/Fe]LTE (=0, 0.2 and 0.4 in the first, second and third row respectively), between two stars with Teff/log g parameters shown at the bottom right of each plot. The LTE difference Δ[Mg/Fe]LTE is represented by the dotted line. Colours indicate the LTE abundance [Mg/Fe]LTE for each star shown at the top-left of each plot. Four different Mg i lines were used: 5711(Λ), 7691(), 5528 () and 8806 () Å. Examples of individual stars at various evolutionary stages were selected: main sequence (MS), turn off point (TOP), red giant branch (RGB) and base of the RGB (bRGB).

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