377 citations · 2.4k across the 34 of their papers we have counts for
6 papers · 1 filter
Observable tests of self-interacting dark matter in galaxy clusters: BCG wobbles in a constant density core
David Harvey, Andrew Robertson, Richard Massey +1
Models of Cold Dark Matter predict that the distribution of dark matter in galaxy clusters should be cuspy, centrally concentrated. Constant density cores would be strong evidence…
The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE
Adrien C. R. Thob, Robert A. Crain, Ian G. McCarthy +7
We investigate the connection between the morphology and internal kinematics of the stellar component of central galaxies with mass in the EAGL…
The gas fractions of dark matter haloes hosting simulated galaxies are governed by the feedback history of their black holes
Jonathan J. Davies, Robert A. Crain, Ian G. McCarthy +4
We examine the origin of scatter in the relationship between the gas fraction and mass of dark matter haloes hosting present-day central galaxies in the EAGLE simula…
Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons
Andrew Robertson, David Harvey, Richard Massey +5
We present BAHAMAS-SIDM, the first large-volume, (400/h Mpc)^3, cosmological simulations including both self-interacting dark matter (SIDM) and baryonic physics. These simulations…
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…
Prospects for Determining the Mass Distributions of Galaxy Clusters on Large Scales Using Weak Gravitational Lensing
M. Fong, R. Bowyer, A. Whitehead +4
For more than two decades, the Navarro, Frenk, and White (NFW) model has stood the test of time; it has been used to describe the distribution of mass in galaxy clusters out to the…