activity
20122026
most citedConcurrent formation of supermassive stars and globular clusters: implications for early self-enrichment

220 citations · 1.3k across the 37 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2020★ 7 cited

The proper motion of sub-populations in Omega Centauri

N. Sanna, E. Pancino, A. Zocchi +2

The galactic globular cluster Omega Centauri is the most massive of its kind, with a complex mix of multiple stellar populations and several kinematic and dynamical peculiarities.…

astro-ph.SR2020★ 19 cited

The not so simple stellar system Omega Cen. II. Evidence in support of a merging scenario

Annalisa Calamida, Alice Zocchi, Giuseppe Bono +7

We present multi-band photometry covering 5° 5°across Cen collected with the Dark Energy Camera, combined to Hubble Space Telescope and Wide Field Imager data fo…

astro-ph.SR2019★ 137 cited

Homogeneous photometry VII. Globular clusters in the Gaia era

P. B. Stetson, E. Pancino, A. Zocchi +2

We present wide-field, ground-based Johnson-Cousins UBVRI photometry for 48 Galactic globular clusters based on almost 90000 public and proprietary images. The photometry is calibr…

astro-ph.SR2018★ 45 cited

The Peculiar Radial Distribution of Multiple Populations in the massive globular cluster M80

E. Dalessandro, M. Cadelano, E. Vesperini +7

We present a detailed analysis of the radial distribution of light-element multiple populations (LE-MPs) in the massive and dense globular cluster M80 based on the combination of U…

astro-ph.SR2016★ 49 cited

The properties of energetically unbound stars in stellar clusters

Ian Claydon, Mark Gieles, Alice Zocchi

Several Milky Way star clusters show a roughly flat velocity dispersion profile at large radii, which is not expected from models with a tidal cut-off energy. Possible explanations…

astro-ph.SR2015

Biases in the determination of dynamical parameters of star clusters: today and in the Gaia era

A. Sollima, H. Baumgardt, A. Zocchi +4

The structural and dynamical properties of star clusters are generally derived by means of the comparison between steady-state analytic models and the available observables. With t…