activity
20242026
collaborators

5 papers

astro-ph.GA2026

Ancient relic moderately metal-rich bulge cluster Tonantzintla 2

Sergio Ortolani, Stefano O. Souza, Domenico Nardiello +6

The assembly history of the Galactic bulge is intimately tied to the formation of the proto-Milky Way, yet reconstructing this early phase is difficult because mergers and secular…

astro-ph.GA2025

The Spheroidal Bulge of the Milky Way: Chemodynamically Distinct from the Inner-Thick Disc and Bar

Samir Nepal, Cristina Chiappini, Angeles Pérez-Villegas +7

Studying the composition and origin of the inner region of our Galaxy -- the "Galactic bulge" -- is crucial for understanding the formation and evolution of the Milky Way and other…

astro-ph.GA2025

The VISCACHA Survey: XIII. The extended main-sequence turn-off in intermediate-age low-mass clusters

Stefano Souza, Angeles Pérez-Villegas, Bruno Dias +16

The extended main-sequence turn-off (eMSTO) is a well-known feature observed in young and intermediate-age star clusters, characterized by a significant broadening of the main-sequ…

astro-ph.GA2025

Revisited parameters for the twin bulge globular clusters NGC 6528 and NGC 6553

S. Ortolani, S. O. Souza, D. Nardiello +2

NGC 6528 and NGC 6553 are among the most metal-rich globular clusters in the Galactic bulge. They represent the upper end of the chemical enrichment in the Galaxy, and can inform o…

astro-ph.GA2024

Tracing back a second-generation star stripped from Terzan 5 by the Galactic bar

Stefano O. Souza, Marica Valentini, Cristina Chiappini +6

The Galactic bulge hosts the Milky Way's oldest stars, possibly coming from disrupted globular clusters (GCs) or the bulge's primordial building blocks, making these stars witnesse…