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Chemical Fingerprints of Accreted Ultrafaint Dwarf Galaxies in the Milky Way Halo

  • Authors: Diala M. Taneenah, Yuqin Chen, Gang Zhao, Motasem J. Alslaihat, Xinyu Wang, Renjing Xie, Haining Li

Diala M. Taneenah et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 1.

Left: distribution of the sample star in the [Ba/Fe]–[Sr/Ba] plane. The solid black line shows the selection boundary, [Sr/Ba] = −0.8[Ba/Fe] − 0.7, and the dashed lines indicate the ±0.2 dex uncertainty band. Right: histogram of the signed offset from the selection boundary, Δcut = [Sr/Ba] + 0.8[Ba/Fe] + 0.7. The dashed line marks the adopted division at Δcut = 0, separating the low-[Sr/Ba] stars from the rest of the sample.

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