We investigate the relationship between stellar and gas specific angular momentum j, stellar
mass M* and optical morphology for a sample of 488 galaxies extracted from the Sydney …

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 …

Abstract We apply the Jeans Anisotropic Multi-Gaussian Expansion dynamical modelling
method to SAGES Legacy Unifying Globulars and GalaxieS (SLUGGS) survey data of early …

Context. Lenticular (S0) galaxies are known to derive from spiral galaxies. The fact that S0s
nearly obey the Tully-Fisher relation (TFR) at z~ 0 (as spirals have done in the last~ 9 Gyr) is …

Lenticular galaxies are generally thought to have descended from spirals via morphological
transformation, although recent numerical simulations have shown that minor or even major …

The CALIFA team has recently found that the stellar angular momentum and concentration
of late-type spiral galaxies are incompatible with those of lenticular galaxies (S0s) …

We present a detailed analysis of a large sample of spectroscopically confirmed massive
quiescent galaxies (MQGs; log (M*/M⊙)∼ 11.5) at z≳ 2. This sample comprises 15 galaxies …

The removal of the interstellar medium (ISM) of disc galaxies through ram pressure stripping
(RPS) has been extensively studied in numerous simulations. Nevertheless, the role of …

Context. Lenticular galaxies (S0s) are more likely to host antitruncated (Type III) stellar discs
than galaxies of later Hubble types. Major mergers are popularly considered too violent to …

Context. Observations reveal a strong structural coupling between bulge and disc in S0
galaxies, which seems difficult to explain if they have formed from supposedly catastrophic …