Robles et al., available on arXiv. Abstract: We compare a suite of four simulated dwarf galaxies formed in 10^10 Msun haloes of collisionless Cold Dark …
Ma et al., available on arXiv. Abstract: We present a suite of cosmological zoom-in simulations at z>5 from the Feedback In Realistic Environments project, spanning …
Gonzalez-Samaniego et al., available on arXiv. Abstract: We use a suite of high-resolution cosmological dwarf galaxy simulations to test the accuracy of commonly-used mass estimators …
El Badry et al., available on arXiv. Abstract: We study the z=0 gas kinematics, morphology, and angular momentum content of isolated galaxies in a suite …
van de Voort et al., available on arXiv. Abstract: We quantify the gas-phase abundance of deuterium in cosmological zoom-in simulations from the Feedback In Realistic …
Kim et al., available on arXiv. Abstract: Using a state-of-the-art cosmological simulation of merging proto-galaxies at high redshift from the FIRE project, with explicit treatments …
Hopkins et al., available on arXiv. Abstract: The Feedback In Realistic Environments (FIRE) project explores the role of feedback in cosmological simulations of galaxy formation. …
Garrison-Kimmel et al., available on arXiv. Abstract: Among the most important goals in cosmology is detecting and quantifying small (M_halo ~ 10^6-9 Msun) dark matter …
Orr et al., available on arXiv. Abstract: We present an analysis of the global and spatially-resolved Kennicutt-Schmidt star formation relation in the FIRE (Feedback In …
Grudić et al., available on arXiv. Abstract: We present a suite of 3D multi-physics MHD simulations following star formation in isolated turbulent molecular gas disks …