Su et al, available on arXiv Abstract: Using high-resolution simulations from the FIRE-2 (Feedback In Realistic Environments) project, we study the effects of discreteness in …
Chan et al., available on arXiv Abstract: We test if the cosmological zoom-in simulations of isolated galaxies from the FIRE project reproduce the properties of …
Escala et al., available at Abstract: We investigate stellar metallicity distribution functions (MDFs), including Fe and α-element abundances, in dwarf galaxies from the Feedback in …
Su et al., available on arXiv Abstract: Using high-resolution magnetohydrodynamic simulations of idealized, non-cosmological galaxies, we investigate how cooling, star formation, and stellar feedback affect …
Ma et al., available on arXiv Abstract: We study the morphologies and sizes of galaxies at z>5 using high-resolution cosmological zoom-in simulations from the Feedback …
Orr et al., available on arXiv Abstract: In a recent work based on 3200 stacked Hα maps of galaxies at z~1, Nelson et al. find …
Hopkins et al., available on arXiv. Abstract: We study the implementation of mechanical feedback from supernovae (SNe) and stellar mass loss in galaxy simulations, within …
Angles-Alcazar et al., available on arXiv. Abstract: We introduce massive black holes (BHs) in the Feedback In Realistic Environments project and perform high-resolution cosmological hydrodynamic …
Hopkins et al., available on arXiv. Abstract: We study the implementation of mechanical feedback from supernovae (SNe) and stellar mass loss in galaxy simulations, within …
Price et al., available on arXiv. Abstract: Accurate measurements of galaxy masses and sizes are key to tracing galaxy evolution over time. Cosmological zoom-in simulations …