We present a novel framework to self-consistently model the effects of radiation fields, dust
physics, and molecular chemistry (H2) in the interstellar medium (ISM) of galaxies. The …

Context. Low-metallicity dwarf galaxies often show no or little CO emission, despite the
intense star formation observed in local samples. Both simulations and resolved …

We present the first nonparametric morphological analysis of a set of spiral galaxies from UV
to submillimeter (submm) wavelengths. Our study is based on high-quality multi-wavelength …

Power spectra of deprojected images of late-type galaxies in gas or dust emission are very
useful diagnostics of the dynamics and stability of their interstellar medium. Previous studies …

Context. Within the framework of the HERM33ES key program, we are studying the star
forming interstellar medium in the nearby, metal-poor spiral galaxy M 33, exploiting the high …

Context. We have obtained Herschel images at five wavelengths from 100 to 500 μm of a~
5.5× 2.5 degree area centred on the local galaxy M 31 (Andromeda), our nearest neighbour …

We present a high spatial resolution study, on scales of∼ 100 pc, of the relationship
between star formation rate (SFR) and gas content within Local Group galaxy M33 …

We utilize archival far-infrared maps from the Herschel Space Observatory in four Local
Group galaxies (Small and Large Magellanic Clouds (SMC and LMC), M31, and M33). We …

We study the wavelength dependence of the dust emission as a function of position and
environment across the disk of M 33 using Spitzer and Herschel photometric data. M 33 is a …

We have conducted a near-infrared monitoring campaign at the UK Infrared Telescope of
the Local Group spiral galaxy M 33 (Triangulum). On the basis of their variability, we have …