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Characterizing the Velocity Anisotropy of the Milky Way’s Stellar Halo

  • Authors: F. O. Barbosa, A. Pérez-Villegas, S. Rossi, R. M. Santucci, L. Aguilar, H. D. Perottoni, G. Limberg, L. Borbolato, J. V. Nogueira-Santos

F. O. Barbosa et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 7.

Anisotropy profiles for color bins dividing the complete (top panel) and clean sample ([Fe/H] > −1.8, middle panel; and [Fe/H] < −1.8, bottom panel). Color bins are indicated by color and thickness. The lines correspond to the median values and the respective bands indicate the limits using 16th and 84th percentiles obtained with MC simulation.

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