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Moving mesh cosmology: tracing cosmological gas accretion

Monthly Notices of the Royal Astronomical Society, no. 4 (2013): 3353-3370

Cited: 92|Views25

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methods: numericalgalaxies: evolutiongalaxies: formationgalaxies: haloescosmology: theory

Abstract

We investigate the nature of gas accretion on to haloes and galaxies at z = 2 using cosmological hydrodynamic simulations run with the moving mesh code AREPO. Implementing a Monte Carlo tracer particle scheme to determine the origin and thermodynamic history of accreting gas, we make quantitative comparisons to an otherwise identical simu...More

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dylan nelson

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