activity
19952023
most citedA consistent explanation for C/C, Li, and He anomalies in red giant stars

307 citations · 781 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2023

C/C of Kepler giant stars: the missing piece of the mixing puzzle

N. Lagarde, R. Minkeviciute, A. Drazdauskas +6

Despite a rich observational background, few spectroscopic studies have dealt with the measurement of the carbon isotopic ratio in giant stars. However, it is a key element in unde…

astro-ph.SR2010★ 4 cited

Observational signatures of lithium depletion in the metal-poor globular cluster NGC6397

K. Lind, F. Primas, C. Charbonnel +2

The "stellar" solution to the cosmological lithium problem proposes that surface depletion of lithium in low-mass, metal-poor stars can reconcile the lower abundances found for Gal…

astro-ph.SR2010★ 2 cited

Beryllium abundances along the evolutionary sequence of the open cluster IC 4651

Rodolfo Smiljanic, L. Pasquini, C. Charbonnel +1

The simultaneous investigation of Li and Be in stars is a powerful tool in the study of the evolutionary mixing processes. Here, we present beryllium abundances in stars along the…

astro-ph.SR2009★ 35 cited

Beryllium abundances along the evolutionary sequence of the open cluster IC 4651 - New test for hydrodynamical stellar models

Rodolfo Smiljanic, Luca Pasquini, Corinne Charbonnel +1

[abridged] Previous analyses of lithium abundances in main sequence and red giant stars have revealed the action of mixing mechanisms other than convection in stellar interiors. Be…

astro-ph2008★ 113 cited

CNONa and 12C/13C in giants of 10 open clusters

R. Smiljanic, R. Gauderon, P. North +3

Evolved low-mass stars of a wide range of metallicity bear signatures of a non-standard mixing event in their surface abundances of Li, C, and N, and in their 12C/13C ratio. A Na o…

astro-ph2004★ 107 cited

Detailed chemical composition of the open cluster IC 4651: The iron peak, alpha elements, and Li

L. Pasquini, S. Randich, M. Zoccali +3

We present a detailed chemical analysis of 22 stars along the colour-magnitude sequence of the intermediate-age (1.7 Gyr) open cluster IC 4651. We find for the cluster a well-defin…