Fig. 8
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Mean abundances of NGC 362 and NGC 1261 derived in this work (the colour coding is the same as in Fig. 3) compared with those of GSE stars (grey filled points, either derived in this work or by Ceccarelli et al. (2024) for Mg, Ca, TiI, Zn, and YII). Literature abundances for [EuII/Fe] are taken from Fishlock et al. (2017); Aguado et al. (2021); Carrillo et al. (2022); Giribaldi & Smiljanic (2023); François et al. (2024). Error bars stand for the standard deviation.
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