Related references
Note: Only part of the references are listed.Probing the shape and history of the Milky Way halo with orbital spectral analysis
Monica Valluri et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2012)
A halo expansion technique for approximating simulated dark matter haloes
Ben Lowing et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)
The density and pseudo-phase-space density profiles of cold dark matter haloes
Aaron D. Ludlow et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)
The drop in the cosmic star formation rate below redshift 2 is caused by a change in the mode of gas accretion and by active galactic nucleus feedback
Freeke van de Voort et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)
The correlation structure of dark matter halo properties
Akila Jeeson-Daniel et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)
ORBITAL STRUCTURE OF MERGER REMNANTS. I. EFFECT OF GAS FRACTION IN PURE DISK MERGERS
Loren Hoffman et al.
ASTROPHYSICAL JOURNAL (2010)
The diversity and similarity of simulated cold dark matter haloes
Julio F. Navarro et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2010)
The orbital evolution induced by baryonic condensation in triaxial haloes
Monica Valluri et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2010)
The physics driving the cosmic star formation history
Joop Schaye et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2010)
ACCURATE UNIVERSAL MODELS FOR THE MASS ACCRETION HISTORIES AND CONCENTRATIONS OF DARK MATTER HALOS
D. H. Zhao et al.
ASTROPHYSICAL JOURNAL (2009)
Tailoring triaxial N-body models via a novel made-to-measure method
Walter Dehnen
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
The effect of photoionization on the cooling rates of enriched, astrophysical plasmas
Robert P. C. Wiersma et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
Substructures in hydrodynamical cluster simulations
K. Dolag et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
C. M. Booth et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
The causes of halo shape changes induced by cooling baryons: Disks versus substructures
Victor P. Debattista et al.
ASTROPHYSICAL JOURNAL (2008)
Disassembling the Galaxy with angle-action coordinates
Paul J. McMillan et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)
Concentration, spin and shape of dark matter haloes as a function of the cosmological model: WMAP1, WMAP3 and WMAP5 results
Andrea V. Maccio et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)
Simulating galactic outflows with kinetic supernova feedback
Claudio Dalla Vecchia et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)
The Aquarius Project: the subhaloes of galactic haloes
V. Springel et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)
On the relation between the Schmidt and Kennicutt-Schmidt star formation laws and its implications for numerical simulations
Joop Schaye et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)
The statistics of Λ CDM halo concentrations
Angelo F. Neto et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
Figure rotation of dark haloes in cold dark matter simulations
S. E. Bryan et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:: Implications for cosmology
D. N. Spergel et al.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2007)
The spin and shape of dark matter haloes in the Millennium simulation of a Λ cold dark matter universe
Philip Bett et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
NMAGIC:: a fast parallel implementation of a χ2-made-to-measure algorithm for modelling observational data
Flavio De Lorenzi et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)
Density profiles of collisionless equilibria. I. Spherical isotropic systems
Eric I. Barnes et al.
ASTROPHYSICAL JOURNAL (2006)
The shape of dark matter haloes: dependence on mass, redshift, radius and formation
B Allgood et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2006)
Radial distribution and strong lensing statistics of satellite galaxies and substructure using high-resolution ΛCDM hydrodynamical simulations
AV Macciò et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2006)
A universal density slope - Velocity anisotropy relation for relaxed structures
SH Hansen et al.
NEW ASTRONOMY (2006)
The cosmological simulation code GADGET-2
V Springel
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2005)
Dynamical insight into dark matter haloes
W Dehnen et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2005)
Internal and external alignment of the shapes and angular momenta of ACDM halos
J Bailin et al.
ASTROPHYSICAL JOURNAL (2005)
Orbital structure of collisionless merger remnants: on the origin of photometric and kinematic properties of elliptical and S0 galaxies
R Jesseit et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2005)
Simulations of the formation, evolution and clustering of galaxies and quasars
V Springel et al.
NATURE (2005)
Figure rotation of cosmological dark matter halos
J Bailin et al.
ASTROPHYSICAL JOURNAL (2004)
Galactic stellar and substellar initial mass function
G Chabrier
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC (2003)
The inner structure of Lambda CDM haloes - I. A numerical convergence study
C Power et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2003)
Triaxial modeling of halo density profiles with high-resolution N-body simulations
YP Jing et al.
ASTROPHYSICAL JOURNAL (2002)
The phase-space density profiles of cold dark matter halos
JE Taylor et al.
ASTROPHYSICAL JOURNAL (2001)
Populating a cluster of galaxies -: I.: Results at z=0
V Springel et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2001)
A universal angular momentum profile for galactic halos
JS Bullock et al.
ASTROPHYSICAL JOURNAL (2001)
Share Paper
