Repositorio de Universidad Autónoma de Chile.
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The central spheroids of Milky Way mass-sized galaxies
We study the properties of the central spheroids located within 10 kpc of the centre of mass of MilkyWay mass-sized galaxies simulated in a cosmological context. The simulated central regions are dominated by stars older than 10 Gyr, mostly formed in situ, with a contribution of ~30 per cent from ac
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