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Greg S. Stinson

Researcher at Max Planck Society

Publications -  19
Citations -  3204

Greg S. Stinson is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 12, co-authored 19 publications receiving 2925 citations. Previous affiliations of Greg S. Stinson include University of Central Lancashire & McMaster University.

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Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows

TL;DR: Hydrodynamical simulations in a framework assuming the presence of CDM and a cosmological constant are reported in which the inhomogeneous interstellar medium is resolved and the analogues of dwarf galaxies—bulgeless and with shallow central dark-matter profiles—arise naturally in these simulations.
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The enrichment of the intergalactic medium with adiabatic feedback - I. Metal cooling and metal diffusion

TL;DR: In this paper, a study of metal enrichment of the intergalactic medium (IGM) using a series of smooth particle hydrodynamics (SPH) simulations is presented, employing models for metal cooling and the turbulent diffusion of metals and thermal energy.
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The dependence of dark matter profiles on the stellar-to-halo mass ratio: a prediction for cusps versus cores

TL;DR: In this article, a suite of 31 simulated galaxies drawn from the MaGICC project were used to investigate the effects of baryonic feedback on the density profiles of dark matter haloes.
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Haloes gone MAD: The Halo-Finder Comparison Project

TL;DR: A detailed comparison of fundamental dark matter halo properties retrieved by a substantial number of different halo finders across a wide range of techniques including friends-of-friends, spherical-overdensity and phase-space-based algorithms is presented.
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A mass-dependent density profile for dark matter haloes including the influence of galaxy formation

TL;DR: In this article, a mass-dependent density profile is proposed to describe the distribution of dark matter within galaxies, which takes into account the stellar-to-halo mass dependence of the response of the dark matter to baryonic processes.