The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …

We present the first direct and unbiased measurement of the evolution of the dust mass
function of galaxies over the past 5 billion years of cosmic history using data from the …

We present a pan-chromatic analysis of an unprecedented sample of 1402 250 μm selected
galaxies at z< 0.5 () from the Herschel-ATLAS survey. We complement our Herschel 100 …

We present high-resolution large-scale observations of the molecular and atomic gas in the
Local Group galaxy M 33. The observations were carried out using the HEterodyne Receiver …

Using new far-infrared imaging from the Herschel Space Observatory with ancillary data
from ultraviolet (UV) to submillimeter wavelengths, we estimate the total emission from dust …

Aims. It is still not understood why star-forming galaxies deviate from the ultraviolet colour-
attenuation relation of starburst galaxies. Previous work and models hint that the role of the …

To study the interstellar medium and the interplay between the atomic and molecular
components in a low-metallicity environment, we present a complete high angular and …

Dust emission is one of the main windows to the physics of galaxies and to star formation as
the radiation from young, hot stars is absorbed by the dust and reemitted at longer …

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 …

We study the far infrared (60–500 μm) colours of late-type galaxies in the Herschel
Reference Survey, a K-band selected, volume limited sample of nearby galaxies. The far …