I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …

Context. The presence of dust in the interstellar medium has profound consequences on the
chemical composition of regions where stars are forming. Recent observations show that …

We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of 86
nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses …

Aims. We present a non-parametric morphology analysis of the stellar continuum and
nebular emission lines for a sample of local galaxies. We explore the dependence of the …

Strong bursts of star formation in galaxies may be triggered either by internal or external
mechanisms. We study the distribution and kinematics of the H i gas in the outer regions of …

ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and
size-limited survey of 2352 nearby galaxies with deep imaging at 3.6 and 4.5 μm. In this …

We present the H i-MaNGA programme of H i follow-up for the Mapping Nearby Galaxies at
Apache Point Observatory (MaNGA) survey. MaNGA, which is part of the Fourth phase of the …

We present redshift-zero synthetic observational data considering dust attenuation and dust
emission for the 30 galaxies of the Auriga project, calculated with the skirt radiative transfer …

We introduce the 'Bluedisk'project, a large programme at the Westerbork Synthesis Radio
Telescope that has mapped the H i in a sample of 23 nearby galaxies with unusually high H …

Testing theories of hierarchical structure formation requires estimating the distribution of
galaxy morphologies and its change with redshift. One aspect of this investigation involves …