activity
20072022
most cited3D hydrodynamic simulations for the formation of the Local Group satellite planes

37 citations · 125 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202237 cited

3D hydrodynamic simulations for the formation of the Local Group satellite planes

Indranil Banik, Ingo Thies, Roy Truelove +5

The existence of mutually correlated thin and rotating planes of satellite galaxies around both the Milky Way (MW) and Andromeda (M31) calls for an explanation. Previous work in Mi…

astro-ph.CO20224 cited

The large-scale structure from non-Gaussian primordial perturbations

G. A. Peña, G. N. Candlish

The late-time effect of primordial non-Gaussianity offers a window into the physics of inflation and the very early Universe. In this work we study the consequences of a particular…

astro-ph.GA201919 cited

Leavers and remainers: Galaxies split by group-exit

Nelvy Choque-Challapa, Rory Smith, Graeme Candlish +2

The disruption of substructure in galaxy clusters likely plays an important role in shaping the cluster population as a significant fraction of cluster galaxies today have spent ti…

astro-ph.GA2018

Consequences of the external field effect for MOND disk galaxies in galaxy clusters

G. N. Candlish, R. Smith, Y. Jaffé +1

Galaxies within galaxy clusters are known to be subject to a wide variety of environmental effects, both gravitational and hydrodynamical. In this study, we examine the purely grav…

astro-ph.GA201532 cited

The difficult early stages of embedded star clusters and the importance of the pre-gas expulsion virial ratio

J. P. Farias, R. Smith, M. Fellhauer +4

We examine the effects of gas-expulsion on initially substructured distributions of stars. We perform N-body simulations of the evolution of these distributions in a static backgro…

astro-ph.GA2015

Simple and accurate modelling of the gravitational potential produced by thick and thin exponential disks

Rory Smith, Chris Flynn, Graeme N. Candlish +2

We present accurate models of the gravitational potential produced by a radially exponential disk mass distribution. The models are produced by combining three separate Miyamoto-Na…