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astro-ph2005
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
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…