activity
20242026
collaborators

10 papers

astro-ph.SR2026

X-shooter spectroscopy of giant stars in the nuclear star cluster

L. Origlia, C. Fanelli, A. Mucciarelli +5

Near-IR spectra of a homogeneous sample of 15 red giants in the Galactic nuclear star cluster, within 1.5 pc of SgrA*, have been acquired with X-shooter at the Very Large Telescope…

astro-ph.GA2026

Reassessing the low- massive sequence stars in Gaia RVS

G. Nandakumar, G. Kordopatis, M. Schultheis +4

Recently, a chemically depleted young massive stellar population was identified using the spectroscopic catalogue of Gaia DR3. To explain its characteristics, a recent enhanced sta…

astro-ph.GA2026

The LEGARE Project. I. Chemical evolution model of the Nuclear Stellar Disc in a Bayesian framework

E. Spitoni, M. Schultheis, F. Matteucci +5

The Nuclear Stellar Disc (NSD) of the Milky Way is a dense, rotating stellar system in the central 200 pc. The NSD is thought to be primarily fuelled by bar-driven gas inflows from…

astro-ph.GA2025

Chemical analysis of the Milky Way's Nuclear Star Cluster: Evidence for a metallicity gradient

M. Schultheis, L. Serrano, B. Thorsbro +5

The Milky Way nuclear star cluster (MWNSC) is located together with its surrounding nuclear stellar disc (MWNSD) in the Galactic centre and they dominate the gravitational potentia…

astro-ph.GA2025

Supergiant GCIRS 22 in the Milky Way Nuclear Star Cluster: Revised alpha abundances

B. Thorsbro, S. Khalidy, R. M. Rich +7

Context: The chemical abundances of alpha-elements in Galactic Centre (GC) supergiants provide key insights into the chemical enrichment and star formation history of the Milky Way…

astro-ph.SR2025

Abundances of P, S, and K in 58 bulge spheroid stars from APOGEE

B. Barbuy, H. Ernandes, A. C. S. Friaça +25

We have previously studied several elements in 58 selected bulge spheroid stars, based on spectral lines in the H-band. We now derive the abundances of the less-studied elements ph…