Image Details
Caption: Figure 5.
Neutron-capture elements abundances for the full Sgr sample. Stars in the Sgr streams are marked with open-face circles (∘), whereas stars in the Sgr core are marked with black-filled circles (•). Literature values from C. J. Hansen et al. (2018) and APOGEE (S. Hasselquist et al. 2017) are shown as transparent blue diamonds. Sgr stars from F. Sestito et al. (2024a) are shown as green diamonds (PIGS IX). Halo stars compiled from JINAbase (A. Abohalima & A. Frebel 2018) are shown as gray dots.
© 2025. The Author(s). Published by the American Astronomical Society.