Fig. 10.
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Behaviour of the iron-element [Sc/Fe], [V/Fe], [Ni/Fe], and [Cu/Fe] abundance ratios as a function of [Fe/H]. Abundances of Galactic field stars are from Reddy et al. (2003, 2006) and Roederer et al. (2014) for all the elements, Gratton et al. (2003) for Sc, V, and Ni, Fulbright (2000) for V and Ni, Adibekyan et al. (2012) for Sc and Ni, Edvardsson et al. (1993), Stephens & Boesgaard (2002) and Bensby et al. (2005) for Ni, and Bihain et al. (2004) and Yan et al. (2015) for Cu. Same symbols as in Fig. 8.
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