Lithium burning in the early stages of stellar evolution

Details Lithium burning in the early stages of stellar evolution Lithium burning in the early stages of stellar evolution

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..435p&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Physics

2

Stellar Evolution, Lithium Burning

Scientific paper

Helioseismology has probably pointed out the important role of an hydrodynamical instability located just below the convective zone in the destruction of the solar lithium during the main sequence. This rotationally induced instability occurs in tachocline region where differential rotation disappears. In order to have a more complete and quantitative view of the general process of lithium destruction, we examine in the present study the way the lithium could be burned in the premainsequence phase for the Sun and young clusters' sunlike-stars. We discuss here the influence of different physical processes and present a scenario of the different stages of destruction.

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