activity
20112023
most citedThe Pisa pre-main sequence tracks and isochrones. A database covering a wide range of Z, Y, mass, and age values

285 citations · 1.4k across the 38 of their papers we have counts for

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Showing 2021Show all

5 papers · 1 filter

astro-ph.SR2021★ 32 cited

Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution

E. Franciosini, E. Tognelli, S. Degl'Innocenti +24

Pre-main sequence models with inflated radii are needed to simultaneously reproduce the colour-magnitude diagram and the lithium depletion pattern in young open clusters. We tested…

astro-ph.SR2021★ 59 cited

The Gaia-ESO Survey: Membership probabilities for stars in 63 open and 7 globular clusters from 3D kinematics

R. J. Jackson, R. D. Jeffries, N. J. Wright +26

Spectroscopy from the final internal data release of the Gaia-ESO Survey (GES) has been combined with Gaia EDR3 to assign membership probabilities to targets observed towards 63 Ga…

astro-ph.GA2021★ 3 cited

Robust statistical tools for identifying multiple stellar populations in globular clusters in the presence of measurement errors. A case study: NGC 2808

G. Valle, M. Dell'Omodarme, E. Tognelli

The finding of multiple stellar populations (MP), defined by patterns in the stellar element abundances, is nowadays considered a distinctive feature of globular clusters. However,…

astro-ph.SR2021★ 8 cited

Theoretical predictions of surface light element abundances in protostellar and pre-Main Sequence phase

E. Tognelli, S. Degl'Innocenti, P. G. Prada Moroni +5

Theoretical prediction of surface stellar abundances of light elements -- lithium, beryllium, and boron -- represents one of the most interesting open problems in astrophysics. As…

astro-ph.SR2021★ 54 cited

The Gaia-ESO survey: Mixing processes in low-mass stars traced by lithium abundance in cluster and field stars

L. Magrini, N. Lagarde, C. Charbonnel +42

We aim to constrain the mixing processes in low-mass stars by investigating the behaviour of the Li surface abundance after the main sequence. We take advantage of the data from th…