AV Kravtsov, S Borgani - Annual Review of Astronomy and …, 2012 - annualreviews.org
Formation of galaxy clusters corresponds to the collapse of the largest gravitationally bound overdensities in the initial density field and is accompanied by the most energetic …
T Shibuya, M Ouchi, Y Harikane - The Astrophysical Journal …, 2015 - iopscience.iop.org
We present the redshift evolution of the galaxy effective radius re obtained from the Hubble Space Telescope (HST) samples of∼ 190,000 galaxies at z= 0–10. Our HST samples …
The rapidly expanding field of galaxy formation lies at the interface between astronomy, particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …
High resolution N-body simulations show that the density profiles of dark matter halos formed in the standard CDM cosmogony can be fit accurately by scaling a simple “universal” …
We use high-resolution N-body simulations to study the equilibrium density profiles of dark matter halos in hierarchically clustering universes. We find that all such profiles have the …
CS Frenk, SDM White - Annalen der Physik, 2012 - Wiley Online Library
Dark matter and cosmic structure Page 1 Ann. Phys. (Berlin) 524, No. 9–10, 507–534 (2012) / DOI 10.1002/andp.201200212 Review Article Dark matter and cosmic structure Carlos S. Frenk …
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 individual dark matter …
HJ Mo, S Mao, SDM White - Monthly Notices of the Royal …, 1998 - academic.oup.com
We study the population of galactic discs expected in current hierarchical clustering models for structure formation. A rotationally supported disc with exponential surface density profile …
We describe the GALFORM semi-analytic model for calculating the formation and evolution of galaxies in hierarchical clustering cosmologies. It improves upon, and extends, the earlier …