Fig. 16.
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Intrinsic spread in iron as a function of the total cluster absolute magnitude Mv (from Harris 1996, 2010 edition), logarithm of the initial mass (from Baumgardt et al. 2018), and IQR[O/Na] (from Carretta 2019), from left to right. In each panel we indicate the Pearson coefficient rP (see text for the significance level). A line connects the two values for NGC 1261 from different studies.
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