activity
19952005
most citedThe heavy elements mixture and the stellar cluster age

1 citations · 1 across the 3 of their papers we have counts for

collaborators

10 papers

astro-ph20051 cited

The heavy elements mixture and the stellar cluster age

S. Degl'Innocenti, P. G. Prada Moroni, B. Ricci

Recent analyses of solar spectroscopic data (see Asplund, Grevesse & Sauval 2004 and references therein) suggest a significative variation of the heavy elements abundance. The chan…

astro-ph2003

The Pisa Evolutionary Library

S. Degl'Innocenti, P. Cariulo, P. G. Prada Moroni +1

We supplement recent evolutionary computations of canonical stellar models (i.e. with inefficient core overshooting) with Z=0.0002, 0.0004, 0.0006, 0.001, 0.004, 0.008 and suitable…

astro-ph2003

Near-Infrared photometry of LMC cluster Reticulum

M. Dall'Ora, G. Bono, J. Storm +11

We present near-infrared (JKs) time series data of the Large Magellanic Cloud (LMC) cluster Reticulum. The observing strategy and data reduction (DAOPHOTII/ALLFRAME) allowed us to…

astro-ph2001

The tricky galactic cluster NGC2420

P. G. Prada Moroni, V. Castellani, S. Degl'Innocenti +1

We discuss the CM diagram of the galactic cluster NGC2420 to the light of current theoretical predictions. By relying on the most recent updating of the physical input, one finds t…

astro-ph2001

The stellar content of the Galaxy: the white dwarf population

M. Cignoni, V. Castellani, S. Degl'Innocenti +2

On the basis of theoretical evolutionary expectations, we develop a Galactic model reproducing star counts and synthetic color-magnitude diagrams of field stars, which include the…

astro-ph2001

RR Lyrae variables in Omega Centauri: a theoretical route

V. Castellani, S. Degl'Innocenti, M. Marconi

We present a theoretical approach to infer information about RR Lyrae variables from the morphology of their light curves. The method, already successfully applied to the field fir…