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The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications
Weiguang Cui, Alexander Knebe, Gustavo Yepes +34
We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study…
How does the stellar disk of the Milky Way get its gas?
Sebastian E. Nuza, Cristina Chiappini, Cecilia Scannapieco +3
In chemodynamical evolution models it is usually assumed that the Milky Way galaxy forms from the inside-out implying that gas inflows onto the disk decrease with galactocentric di…
Gas accretion in Milky Way-like galaxies: temporal and radial dependencies
Sebastian E. Nuza, Cecilia Scannapieco, Cristina Chiappini +3
One of the fundamental assumptions of chemical evolution models (CEMs) of the Milky Way (MW) and other spirals is that higher gas accretion rates are expected in the past, and in t…