We fit the rotation curves of isolated dwarf galaxies to directly measure the stellar mass–halo
mass relation (M⋆–M 200) over the mass range 5× 105≲ M⋆/M⊙≲ 108. By accounting for …

ABSTRACT We introduce the 'Engineering Dwarfs at Galaxy Formation's Edge'(EDGE)
project to study the cosmological formation and evolution of the smallest galaxies in the …

We used 87 high-resolution hydrodynamical cosmological simulations from the NIHAO suite
to investigate the relation between the maximum circular velocity () of a dark matter halo in a …

Aims. We test whether or not realistic analysis techniques of advanced hydrodynamical
simulations can alleviate the Too Big To Fail problem (TBTF) for late-type galaxies. TBTF …

We present the public Monte Carlo photoionization and moving-mesh radiation
hydrodynamics code CMacIonize, which can be used to simulate the self-consistent …

We present a scenario for the formation and the morphology of the arrow-shaped dwarf
irregular galaxy NGC 1427A in the Fornax Cluster. This galaxy shows intriguing stellar and …

We present results from the analysis of WIYN pODI imaging of 23 ultracompact high-velocity
clouds (UCHVCs), which were identified in the ALFALFA H i survey as possible dwarf …

A fundamental question regarding the evolution of dwarf spheroidal galaxies is the
identification of the key physical mechanisms responsible for gas depletion. Here, we focus …

Ultra-compact high velocity clouds (UCHVCs) were identified in the Arecibo Legacy Fast
ALFA (ALFALFA) H i survey as potential gas-bearing dark matter halos. Here we present …

A fundamental question regarding the evolution of dwarf spheroidal galaxies is the
identification of the key physical mechanisms responsible for gas depletion. Here, we focus …