216 citations · 254 across the 4 of their papers we have counts for
4 papers
Origin of the Metallicity Distribution in the Thick Disc
Maider S. Miranda, Kate Pilkington, Brad K. Gibson +9
Aims. Using a suite of cosmological chemodynamical disc galaxy simulations, we assess how (a) radial metallicity gradients evolve with scaleheight; (b) the vertical metallicity gra…
Observationally-Motivated Analysis of Simulated Galaxies
M. S. Miranda, B. A. Macfarlane, B. K. Gibson
The spatial and temporal relationships between stellar age, kinematics, and chemistry are a fundamental tool for uncovering the physics driving galaxy formation and evolution. Obse…
The Lowest Metallicity Stars in the LMC: Clues from MaGICC Simulations
Chris B. Brook, Maider S. Miranda, Brad. K. Gibson +2
Using a cosmological hydrodynamical simulation of a galaxy of similar mass to the Large Magellanic Cloud (LMC), we examine the predicted characteristics of its lowest metallicity p…
Thin disc, Thick Disc and Halo in a Simulated Galaxy
C. B. Brook, G. S. Stinson, B. K. Gibson +8
Within a cosmological hydrodynamical simulation, we form a disc galaxy with sub- components which can be assigned to a thin stellar disc, thick disk, and a low mass stellar halo vi…