Abstract We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their
Environments (EAGLE) project, a suite of hydrodynamical simulations that follow the …

Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust
processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to …

Context. The efficiency of the different processes responsible for the evolution of interstellar
dust on the scale of a galaxy are, to date, very uncertain, spanning several orders of …

We study metal depletion due to dust in the interstellar medium (ISM) to infer the properties
of dust grains and characterize the metal and dust content of galaxies down to low metallicity …

We perform smoothed particle hydrodynamics (SPH) simulations of an isolated galaxy with a
new treatment for dust formation and destruction. To this aim, we treat dust and metal …

We develop a model of dust evolution in a multiphase, inhomogeneous interstellar medium
(ISM) using hydrodynamical simulations of giant molecular clouds in a Milky Way–like spiral …

We present full-volume cosmological simulations, using the moving-mesh code arepo to
study the coevolution of dust and galaxies. We extend the dust model in arepo to include …

The interstellar medium is crucial to understanding the physics of active galaxies and the
coevolution between supermassive black holes and their host galaxies. However, direct gas …

Dust-obscured star formation has dominated the cosmic history of star formation, since z≃ 4.
However, the recent finding of significant amount of dust in galaxies out to z≃ 8 has opened …

Context. The assumption of a gas-to-dust mass ratio γ is a common approach to estimate the
basic properties of molecular clouds, such as total mass and column density of molecular …