Ca II triplet spectroscopy of Small Magellanic Cloud red giants - V. Abundances and velocities for 12 massive clusters

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Fig. 12.

Metallicity as a function of the semimajor axis, a, only for Northern Bridge clusters. Solid lines show the data fits inside and outside the tidal radius. We note that the radial range is smaller than that shown in Figs. 10 and 11.

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