activity
20172021
most citedThe AMBRE Project: chemical evolution models for the Milky Way thick and thin discs

116 citations · 527 across the 9 of their papers we have counts for

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Showing astro-ph.GAShow all

12 papers · 1 filter

astro-ph.GA202155 cited

The Gaia-ESO Survey: Galactic evolution of lithium from iDR6

D. Romano, L. Magrini, S. Randich +31

We exploit the unique characteristics of a sample of open clusters (OCs) and field stars for which high-precision 7Li abundances and stellar parameters are homogeneously derived by…

astro-ph.GA2021

On the effects of the Initial Mass Function on Galactic chemical enrichment

S. Goswami, A. Slemer, P. Marigo +7

There is mounting evidence that the stellar initial mass function (IMF) could extend much beyond the canonical Mi ~100, Msun limit, but the impact of such hypothesis on the chemica…

astro-ph.GA202197 cited

APOGEE DR16: a multi-zone chemical evolution model for the Galactic disc based on MCMC methods

E. Spitoni, K. Verma, V. Silva Aguirre +6

The analysis of the APOGEE DR16 data suggests the existence of a clear distinction between two sequences of disc stars at different Galactocentric distances in the [/Fe] vs. [Fe…

astro-ph.GA202072 cited

Chemical evolution of the Milky Way: constraints on the formation of the thick and thin discs

Marco Palla, Francesca Matteucci, Emanuele Spitoni +2

We study the evolution of Milky Way thick and thin discs in the light of the most recent observational data. In particular, we analyze abundance gradients of O, N, Fe and Mg along…

astro-ph.GA202033 cited

Fluorine in the solar neighborhood: modelling the Galactic thick and thin discs

Valeria Grisoni, Donatella Romano, Emanuele Spitoni +3

We investigate the evolution of the abundance of fluorine in the Milky Way thick and thin discs by means of detailed chemical evolution models compared with recent observational da…

astro-ph.GA202040 cited

On the variation of carbon abundance in galaxies and its implications

Donatella Romano, Mariagrazia Franchini, Valeria Grisoni +3

The trends of chemical abundances and abundance ratios observed in stars of different ages, kinematics, and metallicities bear the imprints of several physical processes that concu…