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20022009
most citedThe evolution of the Galactic metallicity gradient from high-resolution spectroscopy of open clusters

190 citations · 570 across the 7 of their papers we have counts for

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astro-ph2008190 cited

The evolution of the Galactic metallicity gradient from high-resolution spectroscopy of open clusters

Laura Magrini, Paola Sestito, Sofia Randich +1

Open clusters offer a unique possibility to study the time evolution of the radial metallicity gradients of several elements in our Galaxy, because they span large intervals in age…

astro-ph2008109 cited

Open clusters as key tracers of Galactic chemical evolution. III. Element abundances in Berkeley 20, Berkeley 29, Collinder 261, and Melotte 66

P. Sestito, A. Bragaglia, S. Randich +3

Galactic open clusters are since long recognized as one of the best tools for investigating the radial distribution of iron and other metals. We employed FLAMES at VLT to collect U…

astro-ph200841 cited

An assessment of Li abundances in weak-lined and classical T Tauri stars of the Taurus-Auriga association

P. Sestito, F. Palla, S. Randich

Accurate measurements of lithium abundances in young low-mass stars provide an independent and reliable age diagnostics. Previous studies of nearby star forming regions have identi…

astro-ph200740 cited

Tracing mixing in stars: new beryllium observations of the open clusters NGC 2516, Hyades, and M67

S. Randich, F. Primas, L. Pasquini +2

Determinations of beryllium abundance in stars, together with lithium, provide a key tool to investigate the so far poorly understood extra-mixing processes at work in stellar inte…

astro-ph200750 cited

Element abundances in the metal rich open cluster NGC6253

P. Sestito, S. Randich, A. Bragaglia

We have carried out a big FLAMES survey of 10 Galactic open clusters aiming at different goals. One of them is the determination of chemical abundances, in order to put constraints…

astro-ph200617 cited

The effect of heavy element opacity on pre-main sequence Li depletion

P. Sestito, S. Degl Innocenti, P. G. Prada Moroni +1

Recent 3-D analysis of the solar spectrum data suggests a significant change of the solar chemical composition. This may affect the temporal evolution of the surface abundance of l…