Modelling chemical abundance distributions for dwarf galaxies in the Local Group: The impact of turbulent metal diffusion

@article{Escala2018ModellingCA,
  title={Modelling chemical abundance distributions for dwarf galaxies in the Local Group: The impact of turbulent metal diffusion},
  author={Ivanna Escala and Andrew Wetzel and Evan N. Kirby and Philip F. Hopkins and Xiangcheng Ma and Coral Wheeler and Duvsan Kerevs and Claude-Andr{\'e} Faucher-Gigu{\`e}re and Eliot Quataert},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2018},
  volume={474},
  pages={2194-2211}
}
We investigate stellar metallicity distribution functions (MDFs), including Fe and α-element abundances, in dwarf galaxies from the Feedback in Realistic Environment (FIRE) project. We examine both isolated dwarf galaxies and those that are satellites of a Milky Way-mass galaxy. In particular, we study the effects of including a sub-grid turbulent model for the diffusion of metals in gas. Simulations that include diffusion have narrower MDFs and abundance ratio distributions, because diffusion… Expand

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