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19942022
most citedA Universal Density Profile from Hierarchical Clustering

9.9k citations · 75.2k across the 209 of their papers we have counts for

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Showing 2016Show all

11 papers · 1 filter

astro-ph.GA2016★ 86 cited

Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering

Bruno M. B. Henriques, Simon D. M. White, Peter A. Thomas +4

We study the quenching of star formation as a function of redshift, environment and stellar mass in the galaxy formation simulations of Henriques et al. (2015), which implement an…

astro-ph.GA2016★ 120 cited

The globular cluster systems of 54 Coma ultra-diffuse galaxies: statistical constraints from HST data

N. C. Amorisco, A. Monachesi, A. Agnello +1

We use data from the HST Coma Cluster Treasury program to assess the richness of the Globular Cluster Systems (GCSs) of 54 Coma ultra-diffuse galaxies (UDGs), 18 of which have a ha…

astro-ph.GA2016★ 76 cited

Properties of HI discs in the Auriga cosmological simulations

Federico Marinacci, Robert Grand, Rüdiger Pakmor +4

We analyse the properties of the HI gas distribution in the Auriga project, a set of magnetohydrodynamic cosmological simulations performed with the moving-mesh code AREPO and a ph…

astro-ph.GA2016★ 568 cited

The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time

Robert J. J. Grand, Facundo A. Gómez, Federico Marinacci +6

We introduce a suite of thirty cosmological magneto-hydrodynamical zoom simulations of the formation of galaxies in isolated Milky Way mass dark haloes. These were carried out with…

astro-ph.GA2016★ 189 cited

A chronicle of galaxy mass assembly in the EAGLE simulation

Yan Qu, John C. Helly, Richard G. Bower +8

We analyse the mass assembly of central galaxies in the EAGLE hydrodynamical simulations. We build merger trees to connect galaxies to their progenitors at different redshifts and…

astro-ph.GA2016★ 100 cited

Quiescence correlates strongly with directly-measured black hole mass in central galaxies

Bryan A. Terrazas, Eric F. Bell, Bruno M. B. Henriques +3

Roughly half of all stars reside in galaxies without significant ongoing star formation. However, galaxy formation models indicate that it is energetically challenging to suppress…