Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …

Icy grain mantles are the main reservoir of the volatile elements that link chemical processes
in dark, interstellar clouds with the formation of planets and the composition of their …

Here we introduce the interstellar dust modelling framework THEMIS (The Heterogeneous
dust Evolution Model for Interstellar Solids), which takes a global view of dust and its …

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 …

Theoretical models predict that core-collapse supernovae (CCSNe) can be efficient dust
producers (0.1-1.0 M⊙), potentially accounting for most of the dust production in the early …

Aims. We perform a homogeneous analysis of an unprecedented set of spatially resolved
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …

Aims. Within the framework of the DustPedia project we investigate the properties of cosmic
dust and its interaction with stellar radiation (originating from different stellar populations) for …

Aims. The purpose of this work is the characterization of the radial distribution of dust, stars,
gas, and star-formation rate (SFR) in a sub-sample of 18 face-on spiral galaxies extracted …

Aims. In this work, we aim to provide a consistent analysis of the dust properties from metal-
poor to metal-rich environments by linking them to fundamental galactic parameters …