Omega Centauri with phylogenetics

Here, we offer a novel approach to disentangling the complex stellar populations within omega Cen based on phylogenetics methodologies from evolutionary biology. These include the Gaussian Mixture Model and Neighbor-Joining clustering algorithms applied to a set of chemical abundances of omega Cen stellar members.

Instead of using the classical approach in astronomy of grouping them into separate populations, we focused on how the stars are related to each other. We could identify stars that likely formed in globular clusters versus those originating from prolonged in-situ star formation and how these stars interconnect. Our analysis supports the hypothesis that omega Cen might be a nuclear star cluster of a galaxy accreted by the Milky Way with a mass of about 10^9^M_{sun}_.