Ruchti, G R; Read, J I; Feltzing, Sofia; Serenelli, Aldo; McMillan, P; Lind, K; Bensby, T; Bergemann, Maria; Asplund, Martin; Vallenari, A; Monaco, Lorenzo
According to our current cosmological model, galaxies like the Milky Way are expected to experience many mergers over their lifetimes. The most massive of the merging galaxies will be dragged towards the disc plane, depositing stars and dark matter into an accreted disc structure. In this work, we utilize the chemodynamical template developed in Ruchti et al. to hunt for accreted stars. We apply the template to a sample of 4675 stars in the third internal data release from the Gaia-ESO...[Show more]
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