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Cited article:

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Why should models of dwarf galaxy evolution care about the initial mass function at low star-formation rates?

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The effect of ram-pressure stripping on dwarf galaxies

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High-resolution three-dimensional simulations of gas removal from ultrafaint dwarf galaxies

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Simulation of formaldehyde formation during a galaxy collision using vectorized numerical method on Intel Xeon Phi accelerators

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Simulating an isolated dwarf galaxy with multichannel feedback and chemical yields from individual stars

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Numerical Modelling of the Dynamics of the Galactic Halos in the Colliding Galaxies

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A new Intel Xeon Phi accelerated hydrodynamic code for numerical simulations of interacting galaxies

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Mathematical modeling of formation, evolution and interaction of galaxies in cosmological context

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The turbulent destruction of clouds – III. Three-dimensional adiabatic shock–cloud simulations

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