Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium

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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...

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Bibliographic Details
Main Authors:	Meiksin, Avery, Bolton, James S., Tittley, Eric R.
Format:	Article
Published:	Oxford University Press 2014
Subjects:	methods: numerical galaxies: formation intergalactic medium large-scale structure of Universe
Online Access:	https://eprints.nottingham.ac.uk/42507/

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