activity
19962002
most citedNucleosynthesis of light elements inside thermally pulsing AGB stars I: the case of intermediate-mass stars

177 citations · 523 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2002★ 167 cited

Rotational mixing in low-mass stars : I Effect of the mu-gradients in main sequence and subgiant Pop I stars

Ana Palacios, Suzanne Talon, Corinne Charbonnel +1

We present a first set of results concerning stellar evolution of rotating low-mass stars. Our models include fully consistent transport of angular momentum and chemicals due to th…

astro-ph2001★ 51 cited

The Lithium Flash - Thermal instabilities generated by lithium burning in RGB stars

A. Palacios, C. Charbonnel, M. Forestini

We present a scenario to explain the lithium-rich phase which occurs on the red giant branch at the so-called bump in the luminosity function. The high transport coefficients requi…

astro-ph2001★ 87 cited

Galactic chemical evolution of Lithium: interplay between stellar sources"

Claudia Travaglio, Sofia Randich, Daniele Galli +4

In this paper we study the evolution of 7Li in the Galaxy considering the contributions of various stellar sources: type II supernovae, novae, red giant stars, and asymptotic giant…

astro-ph2000★ 39 cited

An internet server for update pre-main sequence tracks of low- and intermediate-mass stars

L. Siess, E. Dufour, M. Forestini

We present new grids of pre-main sequence (PMS) tracks for stars in the mass range 0.1 to 7.0 Msun. The computations were performed for four different metallicities (Z=0.01, 0.02,…

astro-ph1999★ 2 cited

Nucleosynthesis in intermediate mass AGB stars

John Lattanzio, Corinne Charbonnel, Manuel Forestini

We present a summary of the main sites for nucleosynthesis in intermediate mass Asymptotic Giant Branch (AGB) stars. We then discuss some detailed evolutionary models and how these…

astro-ph1997

The Brightest Carbon Stars

Cheryl Frost, Robert Cannon, John Lattanzio +2

It is currently accepted that Hot-Bottom-Burning (HBB) in intermediate-mass asymptotic giant branch (AGB) stars prevents the formation of C~stars. Nevertheless, we present in this…