DASH: a library of dynamical subhalo evolution
The abundance and demographics of dark matter substructure are important for many areas in astrophysics and cosmological N-body simulations have been the primary tool used to investigate them. However, it has recently become clear that the simulations are subject to numerical artefacts, which hamper...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2019-05, Vol.485 (1), p.189-202 |
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Sprache: | eng |
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