Low ionization galaxies and evolution in a pilot survey up to z = 1

This work is the study of the chemical complexity and the physical conditions of the molecular gas in three galaxies with different type of activity, in our sample we have a

The circularized stellar mass density profiles for the galaxies in our sample, comparing them with similar mass SDSS ETGs and the massive compact galaxies in Szomoru et al..

Even the most metal-deficient galaxies in the local universe formed from matter that was already preenriched by a previous star formation episode, and the determination of the

The starburst galaxies from the Lehnert & Heckman (1996) sample have a much lower areal star formation rate. Despite having star-forming regions around 6 times larger on

As a first step in our study, we characterized the mid-IR high-ionization emission lines produced by AGN and star-formation for a large sample of local galaxies, includ- ing

(2010) for nine objects in our sam- ple using optical integral field spectroscopy. These nine objects are mostly spirals or weakly interacting galaxies. They found a higher

& Battaner (1989) performed VI broad-band surface photometry on a sample of 13 Seyfert galaxies; they consider two classes: ‘bulge galaxies’ and ‘disc galaxies’ and found that

We therefore conclude that, even though there seems to be a general belief that abundance ratios depend mostly on stellar yields, these are not the only parameter at work when