Fig. 11.
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Behaviour of the neutron capture-elements [Zr/Fe], [Ba/Fe], and [La/Fe] abundance ratios as a function of [Fe/H]. Abundances of Galactic field stars are from Mishenina et al. (2013) and Roederer et al. (2014) for all the elements, Edvardsson et al. (1993), Fulbright (2000) and Reddy et al. (2003) for Zr and Ba, Burris et al. (2000) and Battistini & Bensby (2016) for Zr and La, Stephens & Boesgaard (2002), Barklem et al. (2005) and Bensby et al. (2005) for Ba.
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