Limits on additional mixing in a stellar interior

Details Limits on additional mixing in a stellar interior Limits on additional mixing in a stellar interior

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..428p&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 428-430. In Russian.

Astronomy and Astrophysics

Astronomy

Convection, Mixing, Stellar Cores, Stellar Evolution, Stellar Interiors, Stellar Luminosity, Stellar Mass

Scientific paper

The observed width of the main sequence for the components of close
binaries is examined. It is found that the mass of the additionally
mixed zone above the convective core does not exceed 20 percent of the
mass of the latter.

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