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- W2513790154 abstract "We investigate the physical properties of the progenitors of today living Milky Way-like galaxies that are visible as Damped Ly Absorption systems and Ly Emitters at higher redshifts (z ≈ 2.3, 5.7). To this aim we use a statistical mergertree approach that follows the formation of the Galaxy and its dwarf satellites in a cosmological context, tracing the chemical evolution and stellar population history of the progenitor halos. The model accounts for the properties of the most metal-poor stars and local dwarf galaxies, providing insights on the early cosmic star-formation. Fruitful links between Galactic Archaeology and more distant galaxies are presented." @default.
- W2513790154 created "2016-09-16" @default.
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- W2513790154 date "2012-01-01" @default.
- W2513790154 modified "2023-09-23" @default.
- W2513790154 title "The infant MilkyWay" @default.
- W2513790154 hasPublicationYear "2012" @default.
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