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Fig. 6
Same as Fig. 5 but for NGC 6752, NGC 6205, NGC 5986, NGC 5904, and NGC 6266. The values for NGC 6752 are from our re-analysis of C13 data, the others are from the literature (see the text) but the adopted solar abundance and the NLTE correction for Na have been homogenized to those we used for our own GCs.
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