activity
20082024
most citedA White Dwarf catalogue from Gaia-DR2 and the Virtual Observatory

142 citations · 1.8k across the 36 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2019★ 64 cited

The Gaia-ESO survey: Calibrating a relationship between Age and the [C/N] abundance ratio with open clusters

G. Casali, L. Magrini, E. Tognelli +51

In the era of large high-resolution spectroscopic surveys, high-quality spectra can contribute to our understanding of the Galactic chemical evolution, providing chemical abundance…

astro-ph.GA2018★ 30 cited

The Gaia-ESO Survey: the N/O abundance ratio in the Milky Way

L. Magrini, F. Vincenzo, S. Randich +31

The abundance ratio N/O is a useful tool to study the interplay of galactic processes, e.g. star formation efficiency, time-scale of infall and outflow loading factor We aim to tra…

astro-ph.GA2018★ 54 cited

The Gaia-ESO Survey: the origin and evolution of s-process elements

L. Magrini, L. Spina, S. Randich +45

Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations, giving important constraints to stell…

astro-ph.GA2017★ 16 cited

The Gaia-ESO Survey: dynamics of ionized and neutral gas in the Lagoon nebula (M8)

F. Damiani, R. Bonito, L. Prisinzano +12

We present a spectroscopic study of the dynamics of the ionized and neutral gas throughout the Lagoon nebula (M8), using VLT/FLAMES data from the Gaia-ESO Survey. We explore the co…

astro-ph.GA2017★ 122 cited

The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young field stars

L. Magrini, S. Randich, G. Kordopatis +44

The spatial distribution of elemental abundances in the disc of our Galaxy gives insights both on its assembly process and subsequent evolution, and on the stellar nucleogenesis of…

astro-ph.GA2016★ 78 cited

The Gaia-ESO Survey: Probes of the inner disk abundance gradient

H. R. Jacobson, E. D. Friel, L. Jilkova +41

The nature of the metallicity gradient inside the solar circle (R_GC < 8 kpc) is poorly understood, but studies of Cepheids and a small sample of open clusters suggest that it stee…