The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …

Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …

Using the cosmological baryonic accretion rate and normal star formation (SF) efficiencies,
we present a very simple model for star-forming galaxies that accounts for the mass and …

We present a budget and accounting of metals in and around star-forming galaxies at z∼ 0.
We combine empirically derived star formation histories with updated supernova and …

We introduce the GALEX Arecibo SDSS Survey (GASS), an on-going large programme that
is gathering high quality H i-line spectra using the Arecibo radio telescope for an unbiased …

Making use of H i 21 cm line measurements from the ALFALFA survey (α. 40) and
photometry from the Sloan Digital Sky Survey (SDSS) and Galaxy Evolution Explorer …

We study the formation of disc galaxies in a fully cosmological framework using adaptive
mesh refinement simulations. We perform an extensive parameter study of the main subgrid …

We use a volume-, magnitude-limited sample of nearby galaxies to investigate the effect of
the environment on the H i scaling relations. We confirm that the H i-to-stellar mass ratio …

We investigate the relationship between stellar mass, metallicity and gas content for a
magnitude-and volume-limited sample of 260 nearby late-type galaxies in different …

We use a sample of close galaxy pairs selected from the Sloan Digital Sky Survey Data
Release 4 (SDSS DR4) to investigate in what environments galaxy mergers occur and how …