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GRASIL-3D: an Implemention of Dust Effects in the SEDs of Simulated Galaxies
R. Domínguez-Tenreiro, A. Obreja, G. L. Granato +5
We introduce a new model for the spectral energy distribution of galaxies, GRASIL-3D, which includes a careful modelling of the dust component of the interstellar medium. GRASIL-3D…
The stellar-to-halo mass relation for Local Group galaxies
C. B. Brook, A. Di Cintio, A. Knebe +4
We contend that a single power law halo mass distribution is appropriate for direct matching to the stellar masses of observed Local Group dwarf galaxies, allowing the determinatio…
MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
Jakob Herpich, Gregory S. Stinson, Andrea V. Macciò +4
We study the effect of warm dark matter (WDM) on hydrodynamic simulations of galaxy formation as part of the Making Galaxies in a Cosmological Context (MaGICC) project. We simulate…
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…
The MaGICC Baryon Cycle: The Enrichment History of Simulated Disc Galaxies
C. B. Brook, G. Stinson, B. K. Gibson +4
Using cosmological galaxy formation simulations from the MaGICC project, spanning more than three magnitudes in stellar mass (~10^7-3x10^{10} Msun), we trace the baryonic cycle of…
The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores
Arianna Di Cintio, Chris B. Brook, Andrea V. Maccio +4
We use 31 simulated galaxies from the MaGICC project to investigate the effects of baryonic feedback on the density profiles of dark matter (DM) haloes. The sample covers a wide ma…