Mixing by internal waves. II. Li and Be depletion rate in low mass main sequence.

Details Mixing by internal waves. II. Li and Be depletion rate in low mass main sequence. Mixing by internal waves. II. Li and Be depletion rate in low mass main sequence.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...305..513m&link_type=abstract

Astronomy and Astrophysics, v.305, p.513

Astronomy and Astrophysics

Astrophysics

45

Stars: Abundances, Diffusion

Scientific paper

In this paper we present the results of lithium and beryllium abundances as a function of spectral type provided by the internal wave diffusion coefficient presented by Montalban (1994). The (Li,T_eff_) curves for Hyades and Praesepe clusters obtained after adding the pre-main sequence burning (D'Antona & Mazzitelli 1994) fit satisfactorily the most recent observational data. The Be abundance is also in good agreement with observational estimations.

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