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20032022
most citedVirial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology

370 citations · 1.8k across the 35 of their papers we have counts for

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Showing 2018Show all

14 papers · 1 filter

astro-ph.GA2018

The Three Hundred Project: The evolution of galaxy cluster density profiles

Robert Mostoghiu, Alexander Knebe, Weiguang Cui +5

Recent numerical studies of the dark matter density profiles of massive galaxy clusters (M) show that their median radial mass density profile rem…

astro-ph.GA2018

Major mergers between dark matter haloes -- II. Profile and concentration changes

Nicole E. Drakos, James E. Taylor, Anael Berrouet +2

Several lines of evidence suggest that as dark matter haloes grow their scale radius increases, and that the density in their central region drops. Major mergers seem an obvious me…

astro-ph.GA2018

Major mergers between dark matter haloes -- I. Predictions for size, shape, and spin

Nicole E. Drakos, James E. Taylor, Anael Berrouet +2

The structural properties of individual dark matter haloes, including shape, spin, concentration, and substructure, are linked to the halo's growth history, but the exact connectio…

astro-ph.GA2018

Reliable mass calculation in spherical gravitating systems

Foivos I. Diakogiannis, Geraint F. Lewis, Rodrigo A. Ibata +3

We present an innovative approach to the methodology of dynamical modelling, allowing practical reconstruction of the underlying dark matter mass without assuming both the density…

astro-ph.GA2018

Quenching timescales of galaxies in the EAGLE simulations

Ruby J. Wright, Claudia del P. Lagos, Luke J. M. Davies +3

We use the \eagle\ simulations to study the connection between the quenching timescale, , and the physical mechanisms that transform star-forming galaxies into passive g…

astro-ph.CO2018

nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts

C. Power, P. J. Elahi, C. Welker +11

Galaxy cluster outskirts mark the transition region from the mildly non-linear cosmic web to the highly non-linear, virialised, cluster interior. It is in this transition region th…