On the dust temperatures of high redshift galaxies
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 …
AuthorClaude-Andre Faucher-Giguere
Dust extinction, dust emission, and dust temperature in galaxies at z>=5: a view from the FIRE-2 simulations
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 …
The galaxy – halo connection in low mass halos
Feldmann et al., available on arXiv Abstract: Properties of galaxies vary systematically with the mass of their parent dark matter halos. This basic galaxy – …
A Predicted Correlation Between Age Gradient and Star Formation History in FIRE Dwarf Galaxies
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 …
Be it therefore resolved: Cosmological Simulations of Dwarf Galaxies with Extreme Resolution
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 …
Dwarf Galaxies in CDM, WDM, and SIDM: Disentangling Baryons and Dark Matter Physics
Fitts et al., available on arXiv Abstract: We present a suite of FIRE-2 cosmological zoom-in simulations of isolated field dwarf galaxies, all with masses of …
Cosmic ray feedback in the FIRE simulations: constraining cosmic ray propagation with GeV gamma-ray emission
Chan et al., available on arXiv Abstract: We present the first results of cosmic ray (CR) feedback implemented in the Feedback In Realistic Environments (FIRE) …
The Origins of the Circumgalactic Medium in the FIRE Simulations
Hafen et al., available on arXiv Abstract: We use a particle tracking analysis to study the origins of the circumgalactic medium (CGM), separating it into …
Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
Su et al., available on arXiv Abstract: The quenching ‘maintenance’ and ‘cooling flow’ problems are important from the Milky Way through massive cluster elliptical galaxies. …
The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
Su et al., available on arXiv Abstract: The quenching ‘maintenance’ and related ‘cooling flow’ problems are important in galaxies from Milky Way mass through clusters. …