There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …

ABSTRACT Dwarf galaxies (M⋆< 109 M⊙) are key drivers of mass assembly in high-mass
galaxies, but relatively little is understood about the assembly of dwarf galaxies themselves …

We investigate the origin of rare star formation in an otherwise red-and-dead population of
S0 galaxies, using spatially resolved spectroscopy. Our sample consists of 120 low redshift …

Gas stripping of spiral galaxies or mergers are thought to be the formation mechanisms of
lenticular galaxies. In order to determine the conditions in which each scenario dominates …

We present a combination of the Schwarzschild orbit-superposition dynamical modelling
technique with the spatially resolved mean stellar age and metallicity maps to uncover the …

We study the role of group infall in the assembly and dynamics of galaxy clusters in ΛCDM.
We select 10 clusters with virial mass M 200∼ 1014 from the cosmological hydrodynamical …

We investigate the kinematic properties of nine nearby early-type galaxies with evidence of
a disc-like component. Three of these galaxies are located in the field, five in the group, and …

We investigate the formation history of massive disc galaxies in hydrodynamical simulation–
the IllustrisTNG, to study why massive disc galaxies survive through cosmic time. 83 …

Many processes have been proposed to explain the quenching of star formation in spiral
galaxies and their transformation into S0s. These processes affect the bulge and disc in …

It is well established that there are at least two main channels to form lenticular (or S0)
galaxies. The first, which we name 'faded spiral'scenario, includes quenching events that led …