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Properties of galaxies reproduced by a hydrodynamic simulation
2014
Nature
Previous simulations of the growth of cosmic structures have broadly reproduced the 'cosmic web' of galaxies that we see in the Universe, but failed to create a mixed population of elliptical and spiral galaxies due to numerical inaccuracies and incomplete physical models. Moreover, because of computational constraints, they were unable to track the small scale evolution of gas and stars to the present epoch within a representative portion of the Universe. Here we report a simulation that
doi:10.1038/nature13316
pmid:24805343
fatcat:2n4oigxgavbpbewd5sdwyl3e6m