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Fig. 1.

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Projected distribution of SMC star clusters from the catalog of Bica et al. (2020) represented by grey dots. Black circles are clusters previously studied with CaT and pink squares clusters studied in this work. Thin dashed lines indicate the ellipses used as a proxy for the distance to the SMC center. The distance a is the semimajor axis of the ellipses indicated in degrees in the figure. The ellipses are tilted by 45° and have an aspect ratio of b/a = 0.5. Thick dashed lines split the regions outside a > 2° into different SMC components. The SMC tidal radius of a = 3.4° (D21) is shown in turquoise.

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