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20082026
most citedGaia Data Release 3: Analysis of RVS spectra using the General Stellar Parametriser from spectroscopy

252 citations · 3.3k across the 91 of their papers we have counts for

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7 papers · 1 filter

astro-ph.SR2026

MINCE IV. A detailed analysis of 37 metal-poor and subsolar metallicity stars

L. Sgatti, G. Cescutti, L. Lombardo +13

The project called Measuring at Intermediate metallicity Neutron-Capture Elements (MINCE) primarily focuses on the photospheric abundances of several neutron-capture (NC) elements…

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.SR2026

The Gaia GSP-Spec catalogue of interstellar extinctions, and stellar luminosities, radii, and masses

Patrick de Laverny, Alejandra Recio-Blanco, Camila Navarrete +2

The Gaia/DR3 GSP-Spec module has published the atmospheric parameters of up to 5.6 million stars based on the analysis of their Radial Velocity Spectrometer spectra. By combining t…

astro-ph.GA2026★ 1 cited

The effects of yields from binary massive stars as functions of metallicity

E. Pepe, E. Spitoni, F. Matteucci +1

Massive stars in binary systems that undergo mass transfer during their lifetime have a different evolution from that of single stars, possibly affecting their chemical yields. Whi…

astro-ph.GA2026

Co-evolution of the Milky Way high- and low-α sequences with chemical evolution models

V. Grisoni, E. Spitoni, F. Matteucci

Observational data have revealed a clear dichotomy in the [α/Fe] vs. [Fe/H] diagram of the Milky Way thick and thin disc stars. Many recent studies have shown evidences of a co-evo…

astro-ph.GA2026★ 2 cited

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…