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Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2011, Volume 415, Issue 3, pp. 2293 - 2318
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 404, Issue 3, pp. 1111 - 1120
...⊙. Within the concordance Λ cold dark matter (ΛCDM) cosmology, the Millennium Simulations give precise halo abundances as a function of mass and redshift for all haloes within which galaxies can form... 
large‐scale structure of Universe | galaxies: luminosity function, mass function | dark matter | galaxies: haloes | cosmology: theory | Galaxies: luminosity function, mass function | Cosmology: theory | Galaxies: haloes | Dark matter | Large-scale structure of Universe | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Galaxies | Analysis | Luminosity | Cosmology | Stars & galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2011, Volume 417, Issue 4, pp. 2982 - 2999
We use a suite of cosmological hydrodynamic simulations to systematically quantify the accretion rates of baryons into dark matter haloes and the resulting baryon mass fractions, as a function of halo... 
galaxies: formation | hydrodynamics | galaxies: evolution | galaxies: high‐redshift | cosmology: theory | Galaxies: evolution | Hydrodynamics | Cosmology: theory | Galaxies: high-redshift | Galaxies: formation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Fluid dynamics | Astronomy | Dark matter | Cosmology | Accretion disks
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2015, Volume 449, Issue 4, pp. 3587 - 3596
... calculation in which DM only interacts gravitationally. Significant differences arise due to the presence of interactions, in terms of the number of low-mass DM haloes and their properties, such as their spin and density profile... 
Galaxies: haloes | Dark matter | Large-scale structure of universe | Astroparticle physics | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Universe | Astrophysics | Radiation | Descriptions | Fluctuation | Nonlinearity | Mathematical models | Formations | Dynamical systems | Density | Cosmology and Extra-Galactic Astrophysics | Physics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 407, Issue 1, pp. 435 - 446
.... Two series of simulations are compared; one that follows only the evolution of the dark matter component of individual haloes in the proper Λcold dark matter (ΛCDM... 
Galaxy: disc | Galaxy: structure | Galaxy: formation | Galaxy: kinematics and dynamics | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Analysis | Astronomy | Astrophysics | Dark matter | Star & galaxy formation | Stars & galaxies | Kinematics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 430, Issue 3, pp. 2346 - 2357
... of the dark matter haloes into which they collect. The initial particle velocities induce central cores in both profiles, which can be understood in the framework of phase-space density theory... 
Dark matter | Galaxies: haloes | Methods: numerical | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Astrophysics | Simulation | Milky Way | Star & galaxy formation | Velocity
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 07/2014, Volume 441, Issue 4, pp. 3359 - 3374
We present the evolution of the structure of relaxed cold dark matter (CDM) haloes in the cosmology from the Planck satellite... 
Cosmology: theory | Galaxies: haloes | Dark matter | Methods: numerical | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Cosmology | Theory | Stars & galaxies | Physics - Cosmology and Nongalactic Astrophysics
Journal Article