The local mixing-length theory with convective helium flux

Details The local mixing-length theory with convective helium flux The local mixing-length theory with convective helium flux

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.150..115u&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 150, no. 1, Dec. 1988, p. 115-147.

Astronomy and Astrophysics

Astrophysics

10

Convective Flow, Helium, Main Sequence Stars, Mixing Length Flow Theory, Chemical Composition, Gas Dynamics, Radiative Heat Transfer, Temperature Gradients

Scientific paper

The local mixing-length theory is extended to calculate distributions of chemical elements in the convective region. There are two different convective solutions in the convective core of the massive Main-Sequence star where convective flux of helium is positive. The condition for the convection to exist with μ-gradient differs from the Ledoux-Sakashita-Hayashi condition when the radiative heat loss from the convective element is taken into account.

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