We summarise recent results from analysis of APOGEE/Gaia data for stellar populations in the Galactic halo, disk, and bulge, leading to constraints on the contribution of dwarf galaxies and globular clusters to the stellar content of the Milky Way halo. Intepretation of the extant data in light of cosmological numerical simulations suggests that the Milky Way has been subject to an unusually intense accretion history at z â 1.5.
|Number of pages||4|
|Journal||Proceedings of the International Astronomical Union|
|Publication status||Published - Feb 2020|
|Event||IAU Symposia: Star Clusters: from the Milky Way to the Early Universe - Bologna, Italy|
Duration: 27 May 2019 → 31 May 2019