Cosmological Gas Accretion Trajectories #1 from halo ita Watch Video
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Description: This visualization shows the trajectories of individual gas elements (on the left) and dark matter particles (on the right) which are bound to the same halo at redshift zero, evolving in time from redshift four. These are extracted from a cosmological hydrodynamical simulation of galaxy formation - part of the moving mesh cosmology project. For more information see http://www.ita.uni-heidelberg.de/~dnelson/
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