Samuel et al., available on arXiv Abstract: The star formation and gas content of satellite galaxies around the Milky Way (MW) and Andromeda (M31) are …
Gurvich et al., available on arXiv Abstract: Recent observations and simulations indicate substantial evolution in the properties of galaxies with time, wherein rotationally-supported and steady …
Hopkins et al., available on arXiv Abstract: Increasingly, uncertainties in predictions from galaxy formation simulations (at sub-Milky Way masses) are dominated by uncertainties in stellar …
Wetzel et al., available on arXiv Abstract: We describe a public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation, available at this …
Bellardini et al., available on arXiv Abstract: We characterize the 3-D spatial variations of [Fe/H], [Mg/H], and [Mg/Fe] in stars at the time of their …
Gandhi et al., available on arXiv Abstract: Type Ia supernovae play a critical role in stellar feedback and elemental enrichment in galaxies. Recent transient surveys …
Moreno et al., available on arXiv Abstract: The standard cold dark matter plus cosmological constant model predicts that galaxies form within dark-matter haloes, and that …
Hafen et al., available on arXiv Abstract: We use FIRE simulations to study disk formation in z~0, Milky Way-mass galaxies, and conclude that a key …
Choban et al., available on arXiv Abstract: Recent strides have been made developing dust evolution models for galaxy formation simulations but these approaches vary in …
Rohr et al., available on arXiv Abstract: Galaxy sizes correlate closely with the sizes of their parent dark matter haloes, suggesting a link between halo …