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Fig. 1.


a: Australian Square Kilometer Array Pathfinder (ASKAP) H I image of the SMC Wing, with the supergiant shell SMC-SGS 1 at its southeastern tip (McClure-Griffiths et al. 2018). b: narrow-band Hα image of SMC-SGS 1 from the Magellanic Cloud Emission-Line Survey (MCELS, Winkler et al. 2005) with regions indicating the photometric field (White), Ramachandran et al. (2019) spectroscopic fields (Yellow), and under-resolved clusters (Blue).

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