Vargya et al., available on arXiv Abstract: Self-interacting dark matter (SIDM) models offer one way to reconcile inconsistencies between observations and predictions from collisionless cold …
Orr et al., available on arXiv Abstract: We examine the azimuthal variations in gas-phase metallicity profiles in simulated Milky Way mass disk galaxies from the …
Porter et al., available on arXiv Abstract: We present an analysis of spatially resolved gas-phase metallicity relations in five dwarf galaxies (Mhalo~10^11 Msun, M*~10^8.8−10^9.6 Msun) …
Shipp et al., available on arXiv Abstract: We present the first detailed study comparing the populations of stellar streams in cosmological simulations to observed Milky …
Shen et al., available on arXiv Abstract: We analyze the first set of cosmological baryonic zoom-in simulations of galaxies in dissipative self-interacting dark matter (dSIDM). …
Shen et al., available on arXiv Abstract: We present the first set of cosmological baryonic zoom-in simulations of galaxies including dissipative self-interacting dark matter (dSIDM). …
Wellons et al., available on arXiv Abstract: Feedback from accreting supermassive black holes (SMBHs) is thought to be a primary driver of quenching in massive …
Grudic et al., available on arXiv Abstract: The properties of young star clusters formed within a galaxy are thought to vary in different interstellar medium …
Rodriguez et al., available on arXiv Abstract: The current generation of galaxy simulations can resolve individual giant molecular clouds, the progenitors of dense star clusters. …
Sameie et al., available on arXiv Abstract: We perform cosmological hydrodynamical simulations to study the formation of proto-globular cluster candidates in progenitors of present-day dwarf …