activity
20032012
most citedThe Origin of the Light Distribution in Spiral Galaxies

159 citations · 450 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2012

RAMSES-CH: A New Chemodynamics Code

C. Gareth Few, Stephanie Courty, Brad K. Gibson

We present a new chemodynamical code based on the adaptive mesh refinement code RAMSES. The new code uses Eulerian hydrodynamics and N-body dynamics in a cosmological framework to…

astro-ph.GA2012★ 51 cited

RAMSES-CH: A New Chemodynamical Code for Cosmological Simulations

C. Gareth Few, Stephanie Courty, Brad K. Gibson +3

We present a new chemodynamical code - Ramses-CH - for use in simulating the self-consistent evolution of chemical and hydrodynamical properties of galaxies within a fully cosmolog…

astro-ph.CO2011★ 27 cited

Observable Signatures of the low-z Circum-Galactic and Inter-Galactic Medium : UV Line Emission in Simulations

S. Frank, Y. Rasera, D. Vibert +8

We present for the first time predictions for UV line emission of intergalactic and circumgalactic gas from Adaptive Mesh Resolution (AMR) Large Scale Structure (LSS) simulations a…

astro-ph.GA2011★ 13 cited

A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models

Owain N. Snaith, Brad K. Gibson, Chris B. Brook +5

Semi-analytic models (SAMs) are currently one of the primary tools with which to model statistically significant ensembles of galaxies. The underlying physical prescriptions inhere…

astro-ph.CO2011★ 70 cited

Disc Heating: Comparing the Milky Way with Cosmological Simulations

Elisa House, Chris B. Brook, Brad K. Gibson +9

We present the analysis of a suite of simulations run with different particle-and grid-based cosmological hydrodynamical codes and compare them with observational data of the Milky…

astro-ph.CO2010★ 4 cited

The circum-galactic gas around cosmologically simulated disks

Stephanie Courty, Brad K. Gibson, Romain Teyssier

We analyze the physical properties and infall rates of the circum-galactic gas around disks obtained in multi-resolved, cosmological, AMR simulations. At intermediate and low redsh…