activity
19992005
most citedThe early evolution of Globular Clusters: the case of NGC 2808

264 citations · 690 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph2005★ 110 cited

Full computation of massive AGB evolution. II. The role of mass loss and cross-sections

Paolo Ventura, Francesca D'Antona

In the course of a systematic exploration of the uncertainties associated to the input micro- and macro-physics in the modeling of the evolution of intermediate mass stars during t…

astro-ph2005★ 57 cited

Helium self--enrichment and the second parameter problem in M3 and M13

V. Caloi, F. D'Antona

Inspection of the CM diagrams of globular clusters having similar heavy element content shows that the luminosity of the red giant bump relative to the turnoff (Delta V_{TO}^{bump}…

astro-ph2004★ 264 cited

The early evolution of Globular Clusters: the case of NGC 2808

Francesca D'Antona, Vittoria Caloi

Enhancement and spread of helium among globular cluster stars have been recently suggested as a way to explain the horizontal branch blue tails, in those clusters which show a prim…

astro-ph2002★ 145 cited

Exploring Brown Dwarf Disks in rho Oph

A. Natta, L. Testi, F. Comeron +5

This paper discusses evidence for and properties of disks associated to brown dwarfs in the star-forming region rho-Oph. We selected nine objects fr om the ISOCAM survey of Bontemp…

astro-ph2001★ 112 cited

Where May Ultra-Fast Rotating Neutron Stars Be Hidden?

L. Burderi, A. Possenti, F. D'Antona +7

The existence of ultra-fast rotating neutron stars (spin period P < 1 ms) is expected on the basis of current models for the secular evolution of interacting binaries, though they…

astro-ph2001★ 2 cited

Lithium and mass loss in massive AGB stars in the Large Magellanic Clouds

P. Ventura, F. D'Antona, I. Mazzitelli

The aim of this work is to use full evolutionary models to derive observational constraints on the mass loss rate of the upper Asymptotic Giant Branch (AGB) stars. The observations…