activity
19992013
most citedCold streams in early massive hot haloes as the main mode of galaxy formation

1.7k citations · 3.2k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.CO2013★ 26 cited

The HST/ACS Coma Cluster Survey - VII. Structure and Assembly of Massive Galaxies in the Center of the Coma Cluster

Tim Weinzirl, Shardha Jogee, Eyal Neistein +16

We constrain the assembly history of galaxies in the projected central 0.5 Mpc of the Coma cluster by performing structural decomposition on 69 massive (M_star >= 10^9 M_sun) galax…

astro-ph.CO2013★ 34 cited

What triggers black-hole growth? Insights from star formation rates

Eyal Neistein, Hagai Netzer

We present a new semi-analytic model for the common growth of black holes (BHs) and galaxies within a hierarchical Universe. The model is tuned to match the mass function of BHs at…

astro-ph.CO2012★ 7 cited

Looking at the relation between haloes and galaxies under the lens

Eyal Neistein, Sadegh Khochfar

We use an empirical approach to model the stellar mass of galaxies according to their host dark-matter haloes and subhaloes ('HASH'), where each galaxy resides in a subhalo taken f…

astro-ph.CO2012★ 246 cited

Ubiquitous seeding of supermassive black holes by direct collapse

Bhaskar Agarwal, Sadegh Khochfar, Jarrett L. Johnson +3

We study for the first time the environment of massive black hole (BH) seeds (~10^4-5 Msun) formed via the direct collapse of pristine gas clouds in massive haloes (>10^7 Msun) at…

astro-ph.CO2011★ 32 cited

Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin

Eyal Neistein, Sadegh Khochfar, Claudio Dalla Vecchia +1

In this work we develop a new method to turn a state-of-the-art hydrodynamical cosmological simulation of galaxy formation (HYD) into a simple semi-analytic model (SAM). This is ac…

astro-ph.CO2011★ 47 cited

A modified star formation law as a solution to open problems in galaxy evolution

Lan Wang, Simone M. Weinmann, Eyal Neistein

In order to reproduce the low mass end of the stellar mass function, most current models of galaxy evolution invoke very efficient supernova feedback. This solution seems to suffer…