Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …

We summarize what large surveys of the contemporary Universe have taught us about the
physics and phenomenology of the processes that link the formation and evolution of …

We introduce the simba simulations, the next generation of the mufasa cosmological galaxy
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …

Context. Water is a key molecule in the physics and chemistry of star and planet formation,
but it is difficult to observe from Earth. The Herschel Space Observatory provided …

Using a large sample of bright nearby stars with accurate Gaia Data Release 2 astrometry
and auxiliary spectroscopy we map out the properties of the principle Galactic components …

We study molecular outflows in a sample of 45 local galaxies, both star forming and active
galactic nucleus (AGN), primarily by using CO data from the Atacama Large Millimeter …

Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …

We study the properties of massive, galactic-scale outflows of molecular gas and investigate
their impact on galaxy evolution. We present new IRAM PdBI CO (1–0) observations of local …

Radiation, winds, and jets from the active nucleus of a massive galaxy can interact with its
interstellar medium, and this can lead to ejection or heating of the gas. This terminates star …

Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the
quenching of massive galaxies in the vast majority of modern galaxy evolution models …