activity
20242026
collaborators

6 papers

astro-ph.GA2026

Globular Clusters in the Time of the JWST. I. Survey Design and First Results on Multiple Populations and Beyond

A. P. Milone, A. F. Marino, G. Cordoni +25

Globular clusters (GCs) host multiple stellar populations with distinct chemical compositions, but their properties among very low-mass stars remain poorly constrained. The James W…

astro-ph.SR2025

A JWST project on 47 Tucanae. Binaries among multiple populations

A. P. Milone, A. F. Marino, M. Bernizzoni +25

Almost all globular clusters (GCs) contain multiple populations consisting of stars with varying helium and light-element abundances. These populations include first-population sta…

astro-ph.GA2025

Linking Photometry and spectroscopy: profiling multiple populations in globular clusters

E. Dondoglio, A. F. Marino, A. P. Milone +14

Our understanding of multiple populations in globular clusters (GCs) largely comes from photometry and spectroscopy: appropriate photometric diagrams can disentangle first and seco…

astro-ph.GA2025

Exploring Multiple Stellar Populations in Globular Clusters with Euclid: A Theoretical Overview and Insights from NGC 6397

A. P. Milone, G. Cordoni, A. F. Marino +8

We investigate the behavior of multiple stellar populations in globular clusters (GCs) using photometric diagrams constructed with Euclid photometry. By employing synthetic spectra…

astro-ph.SR2025

Mass loss along the red giant branch of the intermediate stellar populations in NGC6752 and NGC2808

M. Tailo, A. P. Milone, A. F. Marino +15

The morphology of the Horizontal Branch (HB) in Globular Clusters (GC) is among the early evidences that they contain multiple populations of stars. Indeed, the location of each st…

astro-ph.SR2024

Spectro-Photometry and Radial Distribution of Multiple Stellar Populations in Globular Clusters from Gaia XP Spectra

V. J. Mehta, A. P. Milone, L. Casagrande +14

Understanding the formation of multiple populations in globular clusters (GCs) represents a challenge for stellar population studies. Nevertheless, the outermost cluster regions, l…