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most citedCold streams in early massive hot haloes as the main mode of galaxy formation

1.7k citations · 6.2k across the 22 of their papers we have counts for

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7 papers · 1 filter

astro-ph2006506 cited

Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and Voids

Oliver Hahn, Cristiano Porciani, C. Marcella Carollo +1

Using a series of high-resolution N-body simulations of the concordance cosmology we investigate how the formation histories, shapes and angular momenta of dark-matter haloes depen…

astro-ph2006263 cited

Natural Downsizing in Hierarchical Galaxy Formation

Eyal Neistein, Frank C. van den Bosch, Avishai Dekel

Stellar-population analyses of today's galaxies show "downsizing", where the stars in more massive galaxies tend to have formed earlier and over a shorter time span. We show that t…

astro-ph2006280 cited

A Revised Model for the Formation of Disk Galaxies: Low Spin and Dark-Halo Expansion

Aaron A. Dutton, Frank C. van den Bosch, Avishai Dekel +1

We use observed rotation velocity-luminosity (VL) and size-luminosity (RL) relations to single out a specific scenario for disk galaxy formation in the LCDM cosmology. Our model in…

astro-ph200632 cited

Shapes of Stellar Systems and Dark Halos from Simulations of Galaxy Major Mergers

Gregory S. Novak, Thomas J. Cox, Joel R. Primack +2

Using a sample of 89 snapshots from 58 hydrodynamic binary galaxy major merger simulations, we find that stellar remnants are mostly oblate while dark matter halos are mostly prola…

astro-ph200667 cited

The Dissipative Merger Progenitors of Elliptical Galaxies

Avishai Dekel, Thomas, J. Cox

We address the deviations of the scaling relations of elliptical galaxies from the expectations based on the virial theorem and homology, including the "tilt" of the "fundamental p…

astro-ph2006

Kinematical and Dynamical Modeling of Elliptical Galaxies

G. A. Mamon, E. Lokas, A. Dekel +2

Elements of kinematical and dynamical modeling of elliptical galaxies (Es) are presented. In projection, NFW models resemble Sersic models, but with a very narrow range of shapes (…