Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …

The transformations that take place in late‐type galaxies in the environment of rich clusters
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …

One of the key open questions in extragalactic astronomy is what stops star formation in
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …

Abstract GAs Strip** Phenomena in galaxies with MUSE (GASP) is a new integral-field
spectroscopic survey with MUSE at the VLT aimed at studying gas removal processes in …

Local galaxies are broadly divided into two main classes, star-forming (gas-rich) and
quiescent (passive and gas-poor). The primary mechanism responsible for quenching star …

We provide a census of the apparent stellar angular momentum within one effective radius
of a volume-limited sample of 260 early-type galaxies (ETGs) in the nearby Universe, using …

We extend the phenomenological study of the evolving galaxy population of Peng et
al.(2010) to the central/satellite dichotomy in Yang et al. Sloan Digital Sky Survey (SDSS) …

Exploiting the data from the GAs Strip** Phenomena in galaxies with MUSE (GASP)
program, we compare the integrated star formation rate–mass relation (SFR–M*) relation of …

We present in this paper a detailed analysis of the effect of environment on the star formation
activity of galaxies within the Early Data Release (EDR) of the Sloan Digital Sky Survey …

We have measured the equivalent width of the Hα emission line for 11 006 galaxies brighter
than M b=− 19 (ΩΛ= 0.7, Ω m= 0.3, H 0= 70 km s− 1 Mpc− 1) at 0.05< z< 0.1 in the 2dF …