activity
20242026
collaborators

8 papers

astro-ph.SR2026

Intrinsic iron abundance spreads in globular clusters

J. Schiappacasse-Ulloa, S. Lucatello, L. Magrini +2

Globular Clusters (GCs) host multiple stellar populations, likely composed of a subset of FG stars that enriched the intracluster medium and gave rise to SG stars, each characteris…

astro-ph.IM2025

The WEAVE-TwiLight-Survey: Expanding WEAVE's Reach to Bright and Low-Surface-Density Targets with a Novel Observing Mode

Thomas Hajnik, Nicholas A. Walton, Giuseppe D'Ago +28

Current-day multi-object spectroscopic surveys are often limited in their ability to observe bright stars due to their low surface densities, resulting in increased observational o…

astro-ph.SR2025

Carbon and nitrogen as indicators of stellar evolution and age. A homogeneous sample of 44 open clusters from the Gaia-ESO Survey

G. Tautvaišienė, A. Drazdauskas, Š. Mikolaitis +11

Context. Low- and intermediate-mass giants undergo a complex chemical evolution that has yet to be observationally probed. The influence of core helium flash on the chemical compos…

astro-ph.SR2025

The Gaia-ESO Survey: Projected Rotational Velocities of B stars in the Carina Nebula

W. Santos, S. Daflon, J. V. Sales Silva +19

The Carina Nebula is an active star-forming region with several open clusters rich in massive OB stars, thus making it an optimal target for studying stellar properties such as rot…

astro-ph.GA2025

Neutron-Capture Element Signatures in Globular Clusters: Insights from the Gaia-ESO Survey

J. Schiappacasse-Ulloa, L. Magrini, S. Lucatello +8

Globular clusters (GCs) are key to understanding the formation and evolution of our Galaxy. While the abundances of light and Fe-peak elements in GCs have been widely studied, inve…

astro-ph.GA2025

Inconsistent metallicity spreads in first generation stars of globular clusters from high resolution spectroscopy and HST photometry

Eugenio Carretta, Angela Bragaglia

An open issue about multiple stellar populations in globular clusters (GCs) is the possible existence of metallicity spreads in first generation (FG) stars. Recent estimates based…