Fig. 10.
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Mean abundance ratio of the Fe-peak elements Mn (top) and Ni (bottom) for each of our clusters (filled squares with error bars), compared with APOGEE bulge stars (asterisks – Rojas-Arriagada et al. 2020) and the general trend of disk/halo stars (circles – Reddy et al. 2003, 2006; Battistini & Bensby 2015; Lomaeva et al. 2019). Our BGCs generally follow the bulge field-star trend.
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