Photometric metallicities for 367k stars in Omega Centauri reveal no significant gradient within the half-light radius and well-mixed stellar subpopulations.
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Photometric Metallicities for 367,324 stars of Omega Centauri
Photometric metallicities for 367k stars in Omega Centauri reveal no significant gradient within the half-light radius and well-mixed stellar subpopulations.