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Chemical evolution of galaxies. I. A composition-dependent SPH model for chemical evolution and cooling
Monthly Notices of the Royal Astronomical Society, no. 1 (2008): 39-55
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We describe an smooth particle hydrodynamics (SPH) model for chemical enrichment and radiative cooling in cosmological simulations of structure formation. This model includes: (i) the delayed gas restitution from stars by means of a probabilistic approach designed to reduce the statistical noise and, hence, to allow for the study of the i...更多
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