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 …

This article gives an overview of the constitution, physical conditions, and observables of
dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial …

This paper describes the identification, modelling, and removal of previously unexplained
systematic effects in the polarization data of the Planck High Frequency Instrument (HFI) on …

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 …

Most of the baryons in L* galaxies are unaccounted for and are predicted to lie in hot
gaseous halos (T∼ 10 6.5 K) that may extend beyond R 200. A hot gaseous halo will …

Context. As the millimeter wavelength range remains a largely unexplored spectral region
for galaxies, the IMEGIN large program aims to map the millimeter continuum emission of 22 …

In this first paper in a series we present a study of the global dust emission distribution in
nearby edge-on spiral galaxies. Our sample consists of 16 angularly large and 13 less …

We present new JWST observations of the nearby, prototypical edge-on, spiral galaxy NGC
891. The northern half of the disk was observed with NIRCam in its F150W and F277W …

We present deep far-infrared observations of the nearby edge-on galaxy NGC 891 obtained
with the Herschel Space Observatory and the Spitzer Space Telescope. The maps confirm …

Galaxies are surrounded by halos of hot gas whose mass and origin remain unknown. One
of the most challenging properties to measure is the metallicity, which constrains both of …