Young stellar population gradients in central cluster galaxies from NUV and optical spectroscopy
Central cluster galaxies are the largest and most massive galaxies in the Universe. Although they host very old stellar populations, several studies found the...
Young stellar population gradients in central cluster galaxies from NUV and optical spectroscopy
Central cluster galaxies are the largest and most massive galaxies in the Universe. Although they host very old stellar populations, several studies found the...
z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies. III. Physical properties
The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM Northern Extended Millimeter Array, with the aim to measure their redshift and...
The formation time scales of quiescent galaxies can be estimated in two different ways: by their star formation history and by their chemistry. Previously, the...