activity
19962005
most citedStellar Turbulent Convection: A Selfconsistent Model

298 citations · 354 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2005★ 16 cited

85Peg A: which age for a low metallicity solar like star?

F. D'Antona, D. Cardini, M. P. Di Mauro +3

We explore the possible evolutionary status of the primary component of the binary 85 Pegasi, listed as a target for asteroseismic observations by the MOST satellite. In spite of t…

astro-ph2004

Models of Stellar structure for asteroseismology

F. D'Antona, J. Montalban, I. Mazzitelli

Among the problems still open in the study of stellar structure, we discuss in particular some issues related to the study of convection. We have recently built up complete stellar…

astro-ph1999★ 32 cited

Modeling lithium rich carbon stars in the Large Magellanic Cloud: an independent distance indicator ?

P. Ventura, F. D'Antona, I. Mazzitelli

We present the first quantitative results explaining the presence in the Large Magellanic Cloud of some asymptotic giant branch stars that share the properties of lithium rich carb…

astro-ph1999★ 8 cited

Full spectrum of turbulence convective mixing: II. Lithium production in AGB stars

I. Mazzitelli, F. D'Antona, P. Ventura

We present results from new, detailed computations of lithium production by hot bottom burning (HBB) in asymptotic giant branch (AGB) stars of intermediate mass. The dependance of…

astro-ph1996★ 298 cited

Stellar Turbulent Convection: A Selfconsistent Model

V. M. Canuto, I. Goldman, I. Mazzitelli

We present a selfconsistent model for stellar turbulent convection which is similar in spirit to the CM model (Canuto \& Mazzitelli 1991) since it accounts for the full spectrum of…