Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 9.

Difference between g band (left panels) and r band (right panels) from LAMOST (top panels) and DESI (bottom panels) from SDSS DR16 observations. Median (M) and median absolute deviation (MAD) for each distribution is shown in the top right corner.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse