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The Properties of Globular Clusters and Elqui Associated with the Sagittarius Dwarf Galaxy

  • Authors: P. Wang, W. B. Shi, Y. Q. Chen, J. K. Zhao, J. Zhang, G. Zhao

P. Wang et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 5.

Left panel: the velocity distributions of GCs in the core and stellar stream. The velocity differences between the core and the stellar stream are relatively obvious. Right panel: age as a function of [Fe/H] for the GCs. Under the consideration error, the core is richer than the streams.

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