activity
19982026
most citedAbundance Gradients and the Formation of the Milky Way

688 citations · 4.9k across the 96 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2022★ 9 cited

The Gaia-ESO Survey: Probing the lithium abundances in old metal-rich dwarf stars in the Solar vicinity

M. L. L. Dantas, G. Guiglion, R. Smiljanic +14

We test a scenario in which radial migration could affect the Li abundance pattern of dwarf stars in the solar neighbourhood. This may confirm that the Li abundance in these stars…

astro-ph.SR2021

Gas and dust from extremely metal-poor AGB stars

P. Ventura, F. Dell'Agli, D. Romano +8

We study the evolution of extremely metal-poor AGB stars, with metallicities down to [Fe/H]=-5, to understand the main evolutionary properties, the efficiency of the processes able…

astro-ph.SR2021★ 43 cited

The Gaia-ESO Survey: A new approach to chemically characterising young open clusters II. Abundances of the neutron-capture elements Cu, Sr, Y, Zr, Ba, La, and Ce

M. Baratella, V. D'Orazi, V. Sheminova +32

Young open clusters (t<200 Myr) have been observed to exhibit several peculiarities in their chemical compositions, from a slightly sub-solar iron content, super-solar abundances o…

astro-ph.SR2020★ 14 cited

Stellar population astrophysics (SPA) with the TNG -- The Arcturus Lab

C. Fanelli, L. Origlia, E. Oliva +4

Context. High-resolution spectroscopy in the near-infrared (NIR) is a powerful tool for characterising the physical and chemical properties of cool-star atmospheres. The current ge…

astro-ph.SR2020

Gas and dust from metal-rich AGB stars

Paolo Ventura, Flavia Dell'Agli, Maria Lugaro +3

Context: Stars evolving through the asymptotic giant branch (AGB) phase provide significant feedback to their host system, in form of both gas enriched in nuclear-burning products…

astro-ph.SR2019★ 33 cited

The Gaia-ESO Survey: Carbon abundance in the Galactic thin and thick disks

Mariagrazia Franchini, Carlo Morossi, Paolo Di Marcantonio +24

This paper focuses on carbon that is one of the most abundant elements in the Universe and is of high importance in the field of nucleosynthesis and galactic and stellar evolution.…