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 …

Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …

We demonstrate a novel technology that combines the power of the multi-object
spectrograph with the spatial multiplex advantage of an integral field spectrograph (IFS). The …

We examine the temperature history of gas accreted by forming galaxies in smoothed
particle hydrodynamics simulations. About half of the gas follows the track expected in the …

We use a complete sample of about 140 000 galaxies from the Sloan Digital Sky Survey
(SDSS) to study the size distribution of galaxies and its dependence on their luminosity …

We present the rest-frame colors and luminosities of~ 25,000 m R≲ 24 galaxies in the
redshift range 0.2< z≤ 1.1 drawn from 0.78 deg 2 of the COMBO-17 survey (Classifying …

We measure spectral indexes for 1823 galaxies in the Canadian Network for Observational
Cosmology 1 (CNOC1) sample of 15 X-ray luminous clusters at 0.18< z< 0.55 to investigate …

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 …

The environment is known to affect the formation and evolution of galaxies considerably best
visible through the well-known morphology–density relationship. It is less clear, though …

In Paper I of this series we introduced a volume-limited parent sample of 871 galaxies from
which we extracted the ATLAS3D sample of 260 early-type galaxies (ETGs). In Papers II and …