activity
20172022
most citedThe temporal evolution of neutron-capture elements in the Galactic discs

111 citations · 1k across the 23 of their papers we have counts for

collaborators

40 papers

astro-ph.GA20226 cited

Stellar Population Astrophysics (SPA) with the TNG. alpha-elements, lithium, sodium and aluminum in 16 open clusters

R. Zhang, S. Lucatello, A. Bragaglia +13

Exploring the Galactic chemical evolution and enrichment scenarios with open clusters allows us to understand the history of the Milky Way disk. High-resolution spectra of OCs are…

astro-ph.GA202249 cited

The Gaia-ESO Survey: Age-chemical-clock relations spatially resolved in the Galactic disc

C. Viscasillas Vázquez, L. Magrini, G. Casali +33

The last decade has seen a revolution in our knowledge of the Galaxy thanks to the Gaia and asteroseismic space missions and the ground-based spectroscopic surveys. To complete thi…

astro-ph.GA202266 cited

Mapping the Galactic Metallicity Gradient with Open Clusters: The State-of-the-Art and Future Challenges

Lorenzo Spina, Laura Magrini, Katia Cunha

In this paper, we make use of data collected for open cluster members by high-resolution spectroscopic surveys and programmes (i.e., APOGEE, Gaia-ESO, GALAH, OCCASO, and SPA). Thes…

astro-ph.SR202158 cited

Chemical evidence for planetary ingestion in a quarter of Sun-like stars

Lorenzo Spina, Parth Sharma, Jorge Meléndez +5

Stellar members of binary systems are formed from the same material, therefore they should be chemically identical. However, recent high-precision studies have unveiled chemical di…

astro-ph.SR202126 cited

The Gaia-ESO survey: Lithium abundances in open cluster Red Clump stars

L. Magrini, R. Smiljanic, E. Franciosini +25

It has recently been suggested that all giant stars with mass below 2 suffer an episode of surface lithium enrichment between the tip of the red giant branch (RGB) and…

astro-ph.SR20213 cited

Radial velocity precision of ESPRESSO through the analysis of the solar twin HIP 11915

Yuri Netto, Diego Lorenzo-Oliveira, Jorge Meléndez +4

Different stellar phenomena affect radial velocities (RVs), causing variations large enough to make it difficult to identify planet signals from the stellar variability. RV variati…