Search Results - "White, D. S."
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One simulation to fit them all – changing the background parameters of a cosmological N-body simulation
Published in Monthly notices of the Royal Astronomical Society (11-06-2010)“…We demonstrate that the output of a cosmological N-body simulation can, to remarkable accuracy, be scaled to represent the growth of large-scale structure in a…”
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Universal structure of dark matter haloes over a mass range of 20 orders of magnitude
Published in Nature (London) (03-09-2020)“…Cosmological models in which dark matter consists of cold elementary particles predict that the dark halo population should extend to masses many orders of…”
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The Aquarius Project: the subhaloes of galactic haloes
Published in Monthly notices of the Royal Astronomical Society (21-12-2008)“…We have performed the largest ever particle simulation of a Milky Way sized dark matter halo, and present the most comprehensive convergence study for an…”
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A dynamically cold disk galaxy in the early Universe
Published in Nature (London) (13-08-2020)“…The extreme astrophysical processes and conditions that characterize the early Universe are expected to result in young galaxies that are dynamically different…”
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The physical properties of star-forming galaxies in the low-redshift Universe
Published in Monthly notices of the Royal Astronomical Society (11-07-2004)“…We present a comprehensive study of the physical properties of ∼ 105 galaxies with measurable star formation in the Sloan Digital Sky Survey (SDSS). By…”
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Galactic stellar haloes in the CDM model
Published in Monthly notices of the Royal Astronomical Society (01-08-2010)“…We present six simulations of galactic stellar haloes formed by the tidal disruption of accreted dwarf galaxies in a fully cosmological setting. Our model is…”
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A calibration of the relation between the abundance of close galaxy pairs and the rate of galaxy mergers
Published in Monthly notices of the Royal Astronomical Society (21-12-2008)“…Estimates of galaxy merger rates based on counts of close pairs typically assume that most of the observed systems will merge within a few hundred Myr (for…”
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The high-redshift galaxy population in hierarchical galaxy formation models
Published in Monthly notices of the Royal Astronomical Society (21-03-2007)“…We compare observations of the high-redshift galaxy population to the predictions of the galaxy formation model of Croton et al. and De Lucia & Blaizot. This…”
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Chemodynamics of barred galaxies in cosmological simulations: On the Milky Way’s quiescent merger history and in-situ bulge
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT We explore the chemodynamical properties of a sample of barred galaxies in the Auriga magnetohydrodynamical cosmological zoom-in simulations, which…”
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Scaling relations for galaxy clusters in the Millennium-XXL simulation
Published in Monthly notices of the Royal Astronomical Society (01-11-2012)“…We present a very large high-resolution cosmological N-body simulation, the Millennium-XXL or MXXL, which uses 303 billion particles to represent the formation…”
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The host galaxies of radio-loud active galactic nuclei: mass dependences, gas cooling and active galactic nuclei feedback
Published in Monthly notices of the Royal Astronomical Society (01-09-2005)“…The properties of the host galaxies of a well-defined sample of 2215 radio-loud active galactic nuclei (AGN) with redshifts 0.03 < z < 0.3, defined from the…”
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On the ridges, undulations, and streams in Gaia DR2: linking the topography of phase space to the orbital structure of an N-body bar
Published in Monthly notices of the Royal Astronomical Society (10-07-2019)“…ABSTRACT We explore the origin of phase-space substructures revealed by the second Gaia data release in the disc of the Milky Way, such as the ridges in the…”
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Prospects for detecting supersymmetric dark matter in the Galactic halo
Published in Nature (06-11-2008)“…Dark matter is the dominant form of matter in the Universe, but its nature is unknown. It is plausibly an elementary particle, perhaps the lightest…”
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The Phoenix Project: the dark side of rich Galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (21-09-2012)“…Abstract We introduce the Phoenix Project, a set of Λ cold dark matter (CDM) simulations of the dark matter component of nine rich galaxy clusters. Each…”
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The inner structure of ΛCDM haloes – III. Universality and asymptotic slopes
Published in Monthly notices of the Royal Astronomical Society (11-04-2004)“…We investigate the mass profile of cold dark matter (ΛCDM) haloes using a suite of numerical simulations spanning five decades in halo mass, from dwarf…”
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Feedback and metal enrichment in cosmological SPH simulations – II. A multiphase model with supernova energy feedback
Published in Monthly notices of the Royal Astronomical Society (21-09-2006)“…We have developed a new scheme to treat a multiphase interstellar medium in smoothed particle hydrodynamics simulations of galaxy formation. This scheme can…”
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Limiting performance mechanisms in desiccant wheel dehumidification
Published in Applied thermal engineering (01-11-2012)“…Desiccant cooling is an environmentally attractive alternative to conventional mechanical air-conditioning. The heart of the process is the rotary desiccant…”
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Effects of dark matter substructures on gravitational lensing: results from the Aquarius simulations
Published in Monthly notices of the Royal Astronomical Society (21-09-2009)“…We use the high-resolution Aquarius simulations of the formation of Milky Way-sized haloes in the Λ cold dark matter cosmology to study the effects of dark…”
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The Aquila comparison project: the effects of feedback and numerical methods on simulations of galaxy formation
Published in Monthly notices of the Royal Astronomical Society (01-06-2012)“…We compare the results of various cosmological gas-dynamical codes used to simulate the formation of a galaxy in the Λ cold dark matter structure formation…”
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Feedback and metal enrichment in cosmological smoothed particle hydrodynamics simulations — I. A model for chemical enrichment
Published in Monthly notices of the Royal Astronomical Society (01-12-2005)“…We discuss a model for treating chemical enrichment by Type II and Type Ia supernova (SNII and SNIa) explosions in simulations of cosmological structure…”
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