Thompson et al., available on arXiv Abstract: Our ability to trace the star-forming molecular gas is important to our understanding of the Universe. We can …
Hopkins et al., available on arXiv Abstract: Recently, we demonstrated self-consistent formation of strongly-magnetized quasar accretion disks (QADs) from cosmological radiation-magnetohydrodynamic-thermochemical galaxy-star formation simulations, including …
Hopkins et al., available on arXiv Abstract: In a companion paper, we reported the self-consistent formation of quasar accretion disks with inflow rates ~10 Msun …
Hopkins et al., available on arXiv Abstract: It has recently become possible to zoom-in from cosmological to sub-pc scales in galaxy simulations to follow accretion …
Ponnada et al., available on arXiv Abstract: Synchrotron emission is one of few observable tracers of galactic magnetic fields (B) and cosmic rays (CRs). Much …
Gensior et al., available on arXiv Abstract: Understanding what shapes the cold gas component of galaxies, which both provides the fuel for star formation and …
Shen et al., available on arXiv Abstract: We analyze the first cosmological baryonic zoom-in simulations of galaxies in dissipative self-interacting dark matter (dSIDM). The simulations …
Nguyen et al., available on arXiv Abstract: The third data release (DR3) of Gaia has provided a fivefold increase in the number of radial velocity …
Staudt et al., available on arXiv Abstract: We use FIRE-2 zoom simulations of Milky Way size disk galaxies to derive easy-to-use relationships between the observed …
Graf et al., available on arXiv Abstract: Spatial patterns of stellar elemental abundances encode rich information about a galaxy’s formation history. We analyze the radial, …