Pandya et al., available on arXiv Abstract: We characterize mass, momentum, energy and metal outflow rates of multi-phase galactic winds in a suite of FIRE-2 …
Yu et al., available on arXiv Abstract: We investigate thin and thick stellar disc formation in Milky-Way-mass galaxies using twelve FIRE-2 cosmological zoom-in simulations. All …
Santistevan et al., available on arXiv Abstract: In hierarchical structure formation, metal-poor stars in and around the Milky Way (MW) originate primarily from mergers of …
Parsotan et al., available on arXiv Abstract: The galaxy size-stellar mass and central surface density-stellar mass relationships are observational constraints on galaxy formation models. However, …
Bellardini et al., available on arXiv Abstract: We use FIRE-2 simulations to examine 3-D variations of gas-phase elemental abundances of [O/H], [Fe/H], and [N/H] in …
Flores Velazquez et al., available on arXiv Abstract: Understanding the rate at which stars form is central to studies of galaxy formation. Observationally, the star …
Li et al., available on arXiv Abstract: Observations of UV metal absorption lines have provided insight into the structure and composition of the circumgalactic medium …
Ji et al., available on arXiv Abstract: We study the impact of cosmic rays (CRs) on the structure of virial shocks, using a large suite …
Samuel et al., available on arXiv Abstract: We examine the prevalence, longevity, and causes of planes of satellite dwarf galaxies, as observed in the Local …
Liang et al., available on arXiv Abstract: The relation between infrared excess (IRX) and UV spectral slope (beta_UV) is an empirical probe of dust properties …