Fig. 3.
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[X/Fe] and [Fe/H] abundance kernel density estimation comparison between NGC 2298 (navy blue symbols on the left) and cluster stars (violet, lime green, and cyan symbols for M 53, M 55, and NGC 6397, respectively, on the right) taken from Mészáros et al. (2020). Each violin-type shape indicates the median and limits of the distribution with horizontal lines.
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