activity
20062008
most citedThe fraction of binary systems in the core of thirteen low-density Galactic globular clusters

166 citations · 671 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph200848 cited

The evolution of the binary population in globular clusters: a full analytical computation

A. Sollima

I present a simplified analytical model that simulates the evolution of the binary population in a dynamically evolving globular cluster. A number of simulations have been run span…

astro-ph200870 cited

A Correlation between Blue Straggler and Binary Fractions in the core of Galactic Globular Clusters

A. Sollima, B. Lanzoni, G. Beccari +2

Context. Blue Stragglers Stars (BSSs) are thought to form in globular clusters by two main formation channels: i) mergers induced by stellar collisions and ii) coalescence or mass-…

astro-ph200757 cited

The infrared JHK light curves of RR Lyr

A. Sollima, C. Cacciari, A. A. Arkharov +4

We present infrared JHK time series photometry of the variable star RR Lyr, that allow us to construct the first complete and accurate infrared light curves for this star. The deri…

astro-ph200750 cited

The surprising external upturn of the Blue Straggler radial distribution in M55

B. Lanzoni, E. Dalessandro, S. Perina +4

By combining high-resolution HST and wide-field ground based observations, in ultraviolet and optical bands, we study the Blue Straggler Star (BSS) population of the low density ga…

astro-ph200731 cited

Modeling the chemical evolution of Omega Centauri using three-dimensional hydrodynamical simulations

A. Marcolini, A. Sollima, A. D'Ercole +2

We present a hydrodynamical and chemical model for the globular cluster Omega Cen, under the assumption that it is the remnant of an ancient dwarf spheroidal galaxy (dSph), the bul…

astro-ph200723 cited

The Mass Function of omega Centauri down to 0.15 M_s

A. Sollima, F. R. Ferraro, M. Bellazzini

By means of deep FORS1@VLT and ACS@HST observations of a wide area in the stellar system omega Cen we measured the luminosity function of main sequence stars down to R=22.6 and I_{…