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 …

I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …

MeerKAT's large number (64) of 13.5 m diameter antennas, spanning 8 km with a densely
packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity …

The final product of galaxy evolution through cosmic time is the population of galaxies in the
local universe. These galaxies are also those that can be studied in most detail, thus …

The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

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 present a comprehensive study of the physical properties of∼ 105 galaxies with
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …

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 galaxies drawn from the Sloan Digital Sky Survey to study
how structure, star formation and nuclear activity depend on local density and on stellar …

The study of stellar populations in galaxies is entering a new era with the availability of large
and high-quality data bases of both observed galactic spectra and state-of-the-art …