activity
20152021
most citedWhen the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster

54 citations · 253 across the 13 of their papers we have counts for

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Showing astro-ph.SRShow all

18 papers · 1 filter

astro-ph.SR20218 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

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…

astro-ph.SR202015 cited

On the Metamorphosis of the Bailey diagram for RR Lyrae stars

G. Bono, V. F. Braga, J. Crestani +37

We collected over 6000 high-resolution spectra of four dozen field RR Lyrae (RRL) variables pulsating either in the fundamental (39 RRab) or in the first overtone (9 RRc) mode. We…

astro-ph.SR202010 cited

Protostellar accretion in low mass metal poor stars and the cosmological lithium problem

E. Tognelli, P. G. Prada Moroni, S. Degl'Innocenti +2

The cosmological lithium problem, that is, the discrepancy between the lithium abundance predicted by the Big Bang nucleosynthesis and the one observed for the stars of the 'Spite…

astro-ph.SR2020

Protostellar accretion and the cosmological lithium problem

S. Cassisi, M. Salaris, S. Degl'Innocenti +2

The cosmological lithium problem, i.e. the discrepancy between the lithium abundance predicted by the Big Bang Nucleosynthesis and the one observed for the stars of the "Spite plat…

astro-ph.SR20197 cited

Evidence of a substellar companion to AB Dor C

J. B. Climent, J. P. Berger, J. C. Guirado +5

Studies of fundamental parameters of very low-mass objects are indispensable to provide tests of stellar evolution models that are used to derive theoretical masses of brown dwarfs…