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 …

We study the dust content of galaxies from z= 0 to z= 9 in semi-analytic models of galaxy
formation that include new recipes to track the production and destruction of dust. We …

Context. Current dust models are challenged by the dust properties inferred from the
analysis of Planck observations in total and polarized emission. Aims. We propose new dust …

Abstract The European Space Agency has invested heavily in two cornerstones missions:
Herschel and Planck. The legacy data from these missions provides an unprecedented …

Aims. The DustPedia project is capitalising on the legacy of the Herschel Space
Observatory, using cutting-edge modelling techniques to study dust in the 875 DustPedia …

We study the dust evolution in galaxies by implementing a detailed dust prescription in the
SAGE semi-analytical model (SAM) for galaxy formation. The new model, called Dusty …

Clouds of gas and dust in the Galaxy are nurseries in which stars and planetary systems are
born. During their journey from the diffuse interstellar medium to the protoplanetary disks …

We explore evolution in the dust-to-gas ratio with density within four well-resolved Local
Group galaxies—the LMC, SMC, M31, and M33. We do this using new Herschel maps …

Low-mass protostars are the extrasolar analogues of the natal Solar system. Sophisticated
physicochemical models are used to simulate the formation of two protoplanetary discs from …