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Fig. 8


Relations of the [Al/Fe] ratios in NGC 362 (filled blue squares) from UVES spectra as a function of [Na/Fe] (upper left panel), [Mg/Fe] (upper right), [O/Fe] (lower left panel), and [Si/Fe] (lower right). The star to star error bars are indicated in each panel. As a comparison, the open circles are results for giants in NGC 288 from Carretta et al. (2009b).

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