Non-Standard Mixing in Stars

Details Non-Standard Mixing in Stars Non-Standard Mixing in Stars

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...74..363d&link_type=abstract

Space Science Reviews, Volume 74, Issue 3-4, pp. 363-367

Computer Science

4

Stars, Abundances, Evolution, Rotation, Mixing

Scientific paper

One of the most powerful tests of the stellar evolution theory is analysis of stars' atmospheric chemical composition. It has shown that some non-standard mixing different from ordinary convection, semiconvection and convective overshooting seems to occur in stellar interiors. In the present study Zahn's rotationally induced turbulent diffusion is assumed to be responsible for such kind of mixing. We compare results of our evolutionary calculations with available observational data for massive main-sequence stars and red giants in globular clusters.

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