Fig. 7.
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Comparison between the stellar population present in the central region of the NSD, Sgr B1 (data extracted from Fig. 4 in Nogueras-Lara et al. 2022), and Sgr C (this work). The zoomed-in image shows the youngest age bin, where Sgr B1 and Sgr C show an excess of young stars in comparison to the central region of the NSD.
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