activity
20082016
most citedThe Aquila comparison Project: The Effects of Feedback and Numerical Methods on Simulations of Galaxy Formation

455 citations · 869 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2016★ 79 cited

A Common Origin for Globular Clusters and Ultra-faint Dwarfs in Simulations of the First Galaxies

Massimo Ricotti, Owen H. Parry, Nickolay Y. Gnedin

In this paper, the first in a series on galaxy formation before reionization, we focus on understanding what determines the size and morphology of stellar objects in the first low…

astro-ph.GA2015★ 14 cited

Particle tagging and its implications for stellar population dynamics

Theo Le Bret, Andrew Pontzen, Andrew P. Cooper +5

We establish a controlled comparison between the properties of galactic stellar halos obtained with hydrodynamical simulations and with `particle tagging'. Tagging is a fast way to…

astro-ph.GA2015★ 145 cited

Formation of In Situ Stellar Haloes in Milky Way-Mass Galaxies

Andrew P. Cooper, Owen H. Parry, Ben Lowing +2

We study the formation of stellar haloes in three Milky Way-mass galaxies using cosmological smoothed particle hydrodynamics simulations, focusing on the subset of halo stars that…

astro-ph.GA2011★ 455 cited

The Aquila comparison Project: The Effects of Feedback and Numerical Methods on Simulations of Galaxy Formation

C. Scannapieco, M. Wadepuhl, O. H. Parry +20

We compare the results of thirteen cosmological gasdynamical codes used to simulate the formation of a galaxy in the LCDM structure formation paradigm. The various runs differ in t…

astro-ph.GA2011★ 59 cited

The Baryons in the Milky Way Satellites

Owen H. Parry, Vincent R. Eke, Carlos S. Frenk +1

We investigate the formation and evolution of satellite galaxies using smoothed particle hydrodynamics (SPH) simulations of a Milky Way(MW)-like system, focussing on the best resol…

astro-ph2008★ 117 cited

Galaxy morphology in the LambdaCDM cosmology

O. H. Parry, V. R. Eke, C. S. Frenk

We investigate the origins of galaxy morphology (defined by bulge-to-total K-band luminosity) in the LambdaCDM cosmology using two galaxy formation models ,based on the Millennium…