Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
We perform cosmological simulations of the intergalactic medium (IGM) at redshift z ∼ 3 using the numerical gravity-hydrodynamics codes gadget-3 and enzo for the purpose of modelling the gaseous environments of galaxies. We identify haloes in the simulations using three different algorithms. Differe...
| Main Authors: | , , |
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| Format: | Article |
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Oxford University Press
2014
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| Subjects: | |
| Online Access: | https://eprints.nottingham.ac.uk/42507/ |