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Fig. 4.

image

Distributions of various elemental-abundance ratios from the APOGEE-2 survey for bulge field stars in close proximity to the Galactic Centre (−20° < l < 20° and |b| < 20°), and comparison with stars in NGC 6723. The field-star abundances are represented by orange iso-abundance contours. The member stars of NGC 6723 and the extra-tidal star analyzed in this work are shown with black and red open circles, respectively. The circle sizes reflect their Vo magnitudes, with decreasing size for fainter magnitudes. The blue cross symbol denotes the average ⟨[Xi/Fe]⟩ and its associated star-to-star scatter (σ⟨[Xi/Fe]⟩) of the abundance derived from the seven member NGC 6723 stars analyzed in this work.

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