Hopkins et al, available on arXiv Abstract: We present a suite of high-resolution cosmological simulations, using the FIRE-2 feedback physics together with explicit treatment of …
Garrison-Kimmel et al., available on arXiv Abstract: We present a new set of high-resolution hydrodynamic cosmological zoom-in simulations that apply the Feedback In Realistic Environments …
Cochrane et al., available on arXiv Abstract: We present the first detailed study of the spatially-resolved dust continuum emission of simulated galaxies at z=1-5. We …
Samuel et al., available on arXiv Abstract: While many tensions between Local Group (LG) satellite galaxies and LCDM cosmology have been alleviated through recent cosmological …
Garrison-Kimmel et al., available on arXiv Abstract: We study star formation histories (SFHs) of ~500 dwarf galaxies (stellar mass Mstar = 10^5-10^9 Msun) from FIRE-2 …
Liang et al., available on arXiv Abstract: Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is required when converting …
Ma et al., available on arXiv Abstract: We present a suite of 34 high-resolution cosmological zoom-in simulations consisting of thousands of halos up to M_halo~10^12 …
Feldmann et al., available on arXiv Abstract: Properties of galaxies vary systematically with the mass of their parent dark matter halos. This basic galaxy – …
Graus et al., available on arXiv Abstract: We explore the radial variation of star formation histories in dwarf galaxies simulated with Feedback In Realistic Environments …
Wheeler et al., available on arXiv Abstract: We study a suite of extremely high-resolution cosmological FIRE simulations of dwarf galaxies (M_halo ~ 10^8.6 Msun is …