Image Details

Choose export citation format:

Estimating Accretion Times of Halo Substructures in the Milky Way

  • Authors: Hefan Li, Masashi Chiba, Xiang-Xiang Xue, Gang Zhao

Hefan Li et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 3.

Distributions of the uncertainties in r- and ϕ-direction orbital frequencies for the member stars of the six substructures, with each substructure shown in a different color and marker. The dashed line indicates the 1:1 relation.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse