activity
19982008
most citedIonized gas and stellar kinematics of seventeen nearby spiral galaxies

95 citations · 445 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph2008★ 71 cited

Stellar Populations of Bulges in 14 Cluster Disc Galaxies

L. Morelli, E. Pompei, A. Pizzella +6

Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eridanus and Pegasus cluster, and NGC 7582 group. The structural parameters of the…

astro-ph2008★ 42 cited

Structure and dynamics of galaxies with a low surface brightness disc. I. The stellar and ionised-gas kinematics

A. Pizzella, E. M. Corsini, M. Sarzi +5

(abridged) Photometry and long-slit spectroscopy are presented for a sample of 6 galaxies with a low surface brightness stellar disc and a bulge. The stellar and ionised-gas kinema…

astro-ph2008

The pseudobulge of NGC 1292

L. Morelli, E. Pompei, A. Pizzella +6

The photometric and kinematic properties of Sb NGC 1292 suggest it hosts a pseudobulge. The properties of the stellar population of such a pseudobulge are consistent with a slow bu…

astro-ph2007★ 45 cited

The HELLAS2XMM survey: XI. Unveiling the nature of X-ray Bright Optically Normal Galaxies

F. Civano, M. Mignoli, A. Comastri +8

X-ray Bright Optically Normal Galaxies (XBONGs) constitute a small but not negligible fraction of hard X-ray selected sources in recent Chandra and XMM-Newton surveys. Even though…

astro-ph2006

The chemical evolution of the Milky Way: from light to heavy elements

Francesca Matteucci

We present results for the chemical evolution of the Milky Way including predictions for elements from Deuterium to Europium. A comparison with the most accurate and recent data al…

astro-ph2006★ 20 cited

Cosmic evolution of metal densities: the enrichment of the Inter-Galactic Medium

Francesco Calura, Francesca Matteucci

By means of chemo-photometric models for galaxies of different morhological types, we have carried out a detailed study of the history of element production by spheroidal and dwarf…