Figure 5 from Gaia and Hubble Unveil the Kinematics of Stellar Populations in the Type II Globular Clusters ω Centauri and M22

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Gaia and Hubble Unveil the Kinematics of Stellar Populations in the Type II Globular Clusters ω Centauri and M22

Authors: G. Cordoni, A. P. Milone, A. F. Marino, G. S. Da Costa, E. Dondoglio, H. Jerjen, E. P. Lagioia, A. Mastrobuono-Battisti, J. E. Norris, M. Tailo, and D. Yong

2020 The Astrophysical Journal 898 147.

Provider: AAS Journals

Caption: Figure 5.

Average radial and tangential profile as a function of the radial distance from the cluster centers for ω Centauri (left) and M22 (right). The radial quantity is normalized over the half-light radius from Baumgardt & Hilker (2018). Orange circles and cyan triangles represent Fe-poor and Fe-rich stars, respectively.

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