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Tracing M22’s Origins: Spatial and Chemical Constraints on Its Formation History

  • Authors: Emanuele Dondoglio, Antonino P. Milone, Randa Asa'd, Anna F. Marino, Alessandra Mastrobuono-Battisti, Fabrizio Muratore, Tuila Ziliotto, Emanuele Bortolan, Giacomo Cordoni, Maria Vittoria Legnardi, Edoardo P. Lagioia, Marco Tailo

Emanuele Dondoglio et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 6.

Fraction of canonical and anomalous stars (top) in red and blue, respectively, of 2P stars compared to canonical (middle), and AII with respect to the whole anomalous stars (bottom). Empty dots indicate measurements from HST photometry, while filled dots represent measurement with VST+Gaia (for the bulk of canonical and anomalous) or APOGEE (for the subpopulations). Brown dashed lines indicate the core and half-mass radii from W. E. Harris (1996a, 2010 edition). Each measurement is associated to a horizontal gray line, indicating the reference radial range.

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