Su et al., available on arXiv. Abstract: Using high-resolution simulations with explicit treatment of stellar feedback physics based on the FIRE (Feedback in Realistic Environments) …
Fitts et al., available on arXiv. Abstract: We present a suite of 15 cosmological zoom-in simulations of isolated dark matter halos, all with masses of …
Anglés-Alcázar et al., available on arXiv. Abstract: We use cosmological simulations from the FIRE (Feedback In Realistic Environments) project to study the baryon cycle and …
El-Badry et al., available on arXiv. Abstract: In low-mass galaxies, stellar feedback can drive gas outflows that generate non-equilibrium fluctuations in the gravitational potential. Using …
Ma et al., available on arXiv. Abstract: Recent spatially resolved observations of galaxies at z=0.6-3 reveal that high-redshift galaxies show complex kinematics and a broad …
Feldmann et al., available on arXiv. Abstract: We analyze the SFRs, stellar masses, galaxy colors, and dust extinctions of galaxies in massive (10^12.5-10^13.5 M_sun) halos …
Ma et al., available on arXiv. Abstract: We study the structure, age and metallicity gradients, and dynamical evolution using a cosmological zoom-in simulation of a …
Hafen et al., available on arXiv. Abstract: We use cosmological hydrodynamic simulations with stellar feedback from the FIRE project to study the physical nature of …
Muratov et al., available on arXiv. Abstract: We present an analysis of the flow of metals through the circumgalactic medium in the Feedback in Realistic …
Wetzel et al. report on a new study using a high-resolution simulation of a Milky Way-mass dark matter halo to study the effects of baryonic …