Image Details
Caption: Figure 7.
The SP_Ace code-derived [α/Fe] versus [Fe/H] for the best extratidal candidates selected in Figure 6, Grades A+B (19 objects). The black-filled star marks NGC 6569’s mean values from high-resolution samples (see J18). The open star with error bars is the average of the N. Barrera et al. (2025) sample. Within uncertainties, candidates follow a single locus consistent with NGC 6569; we find no compelling evidence for intrinsic spreads in [Fe/H] or [α/Fe]. A few high-[α/Fe] points occur at low S/N and are treated as upper limits. The gray dots are the Besançon Galactic population models generated for our AAT FOV and PM limits.
© 2026. The Author(s). Published by the American Astronomical Society.