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astro-ph2004

New response functions for absorption-line indices from high-resolution spectra

R. Tantalo, C. Chiosi, L. Piovan

Basing on the huge library of 1-A resolution spectra calculated by Munari et al. over a large range of logT, log g, [Fe/H] and both for solar and a-enhanced abundance ratios [a/Fe]…

astro-ph2002

Kinematics of the disk population in the GAIA era

G. Bertelli, A. Vallenari, S. Pasetto +1

GAIA data will create a precise 3-dimensional map of the Galaxy, providing positional information, radial velocities, luminosity, temperature and chemical composition of a represen…

astro-ph2002

Evolution of zero-metallicity massive stars

P. Marigo, C. Chiosi, L. Girardi +1

We discuss the evolutionary properties of primordial massive and very massive stars, supposed to have formed from metal-free gas. Stellar models are presented over a large range of…

astro-ph2001

A chemical evolution model for galaxy clusters

L. Portinari, A. Moretti, C. Chiosi

We develop a toy-model for the chemical evolution of the intracluster medium, polluted by the galactic winds from elliptical galaxies. The model follows the "galaxy formation histo…

astro-ph2001

Chemical Evolution of Clusters of Galaxies

L. Portinari, A. Moretti, C. Chiosi

The high metallicity of the intra-cluster medium (ICM) is generally interpreted on the base of the galactic wind scenario for elliptical galaxies. In this framework, we develop a t…

astro-ph2000

On radial gas flows, the Galactic Bar and chemical evolution in the Galactic Disc

L. Portinari, C. Chiosi

We develop a numerical chemical model allowing for radial flows of gas, with the aim to analyse the possible role of gas flows in the chemical evolution of the Galactic Disc. The d…