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Cited article:

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edge: the emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations

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Merger-driven Turbulence and Coherent Transport in the Intracluster Medium

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Mixing by internal gravity waves in stars: assessing numerical simulations against theory

J Morton, T Guillet, I Baraffe, A Morison, A Le Saux, D G Vlaykov, T Goffrey and J Pratt
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EDGE – Dark matter or astrophysics? Breaking dark matter heating degeneracies with H i rotation in faint dwarf galaxies

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Hot gas accretion fuels star formation faster than cold accretion in high-redshift galaxies

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The evolution of HCO+ in molecular clouds using a novel chemical post-processing algorithm

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Gravitational torques dominate the dynamics of accreted gas at z > 2

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EDGE: What shapes the relationship between H i and stellar observables in faint dwarf galaxies?

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Stellar angular momentum can be controlled from cosmological initial conditions

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Dynamical heating of the X-ray emitting intracluster medium: the roles of merger shocks and turbulence dissipation

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Monthly Notices of the Royal Astronomical Society 495 (1) 784 (2020)
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Performance optimization of non-equilibrium ionization simulations from MapReduce and GPU acceleration

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Cloud Properties and Correlations with Star Formation in Self-consistent Simulations of the Multiphase ISM

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The nature of strong H i absorbers probed by cosmological simulations: satellite accretion and outflows

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