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

With the advent of the new generation wide-field cameras it became possible to survey in an
unbiased mode galaxies spanning a variety of local densities, from the core of rich clusters …

We investigate the effect of ram-pressure from the intracluster medium on the stripping of H i
gas in galaxies in a massive, relaxed, X-ray bright, galaxy cluster at z= 0.2 from the Blind …

We investigate the velocity versus position phase space of z∼ 1 cluster galaxies using a set
of 424 spectroscopic redshifts in nine clusters drawn from the GCLASS survey. Dividing the …

We present a study of the spatial distribution and kinematics of star-forming galaxies in 30
massive clusters at 0.15< z< 0.30, combining wide-field Spitzer 24 μm and GALEX near …

Star formation is observed to be suppressed in group and cluster galaxies compared to the
field. To gain insight into the quenching process, we have analysed∼ 2000 galaxies formed …

Context. Using MegaCam at the CFHT, we obtained a deep narrow band Hα+[NII] wide-field
image of NGC 4569 (M90), the brightest late-type galaxy in the Virgo cluster. The image …

We study the star formation quenching mechanism in cluster galaxies by fitting the spectral
energy distribution (SED) of the Herschel Reference Survey, a complete volume-limited K …

The Coma cluster is the nearest massive () galaxy cluster, making it an excellent laboratory
to probe the influence of the cluster environment on galaxy star formation. Here, we present …

We present results on the environmental dependence of the star-forming galaxy main
sequence in 11 galaxy cluster fields at 1.0< z< 1.5 from the Gemini Observations of Galaxies …