J. Montalban et E. Schatzman, MIXING BY INTERNAL WAVES .2. LI AND BE DEPLETION RATE IN LOW-MASS MAIN-SEQUENCE, Astronomy and astrophysics, 305(2), 1996, pp. 513-518
In this paper we present the results of lithium and beryllium abundanc
es as a function of spectral type provided by the internal wave diffus
ion coefficient presented by Montalban (1994). The (Li,T-eff) curves f
or Hyades and Praesepe clusters obtained after adding the pre-main seq
uence burning (D'Antona & Mazzitelli 1994) fit satisfactorily the most
recent observational data. The Be abundance is also in good agreement
with observational estimations.