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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 8.

The red dots represent the proper motions of member stars of HSC 61, concentrated at (−2.6874, −1.3126). The red dashed line indicates the average proper motion of the member stars of HSC 61. The gray dots show the distribution of proper motions of field stars in the same sky area as HSC 61.

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