activity
20052026
most citedProbing the properties of convective cores through g modes: high-order g modes in SPB and gamma Doradus stars

254 citations · 984 across the 25 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2026

Stellar ages from [C/N] in giant stars: applicability and limitations

Giada Casali, Luca Casagrande, Fiorenzo Vincenzo +5

The [C/N] abundance ratio is a powerful age indicator for giant stars, enabling age estimates for spectroscopic samples where traditional methods are limited. We calibrate a multiv…

astro-ph.GA2026★ 1 cited

Not all nitrogen-rich field stars originate from globular clusters

Ellen I. Leitinger, Andrea Miglio, Josefina Montalbán +7

Globular clusters (GCs) are important tracers of the early Galactic assembly process, with part of their stars showing distinct chemical abundance patterns. When such stars are fou…

astro-ph.GA2024★ 1 cited

Towards Galactic Archaeology with Inferred Ages of Giant Stars From Gaia Spectra

Aisha S. Almannaei, Daisuke Kawata, Ioana Ciuca +4

In the era of Gaia, the accurate determination of stellar ages is transforming Galactic archaeology. We demonstrate the feasibility of inferring stellar ages from Gaia's RVS spectr…

astro-ph.GA2024★ 33 cited

Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of the Milky Way using Gaia-RVS

Samir Nepal, Cristina Chiappini, Anna B. A. Queiroz +5

JWST has recently detected numerous disc galaxies at high-redshifts and there have been observations of cold disc galaxies at z > 4 with ALMA. In the Milky Way, recent studies find…

astro-ph.GA2023

Insights from Super-Metal-Rich Stars: Is the Milky Way bar young?

Samir Nepal, Cristina Chiappini, Guillaume Guiglion +6

Super-metal-rich (SMR) stars, currently in the solar neighbourhood, are expected to originate only in the inner Galaxy and have definitely migrated. We aim at studying a large samp…

astro-ph.GA2023★ 34 cited

Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) I. The final word on the origin of NGC6388 and NGC6441

Davide Massari, Fernando Aguado-Agelet, Matteo Monelli +11

We present CARMA, the Cluster Ages to Reconstruct the Milky Way Assembly project, that aims at determining precise and accurate age measurements for the entire system of known Gala…