A simplified local mixing-length theory with helium flux and without radiative heat loss from the convective element.

Details A simplified local mixing-length theory with helium flux and without radiative heat loss from the convective element. A simplified local mixing-length theory with helium flux and without radiative heat loss from the convective element.

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990srtoh..10..117u&link_type=abstract

Sci. Rep. Tôhoku Univ., Eighth Ser., Vol. 10, No. 2/3, p. 117 - 122

Physics

1

Massive Stars: Stellar Models, Convection: Stellar Models

Scientific paper

A simplified local mixing-length theory with helium flux and without
radiative heat loss from the convective element is formulated. The
method to construct the massive star models which resemble the models of
Sakashita and Hayashi from the stand point of Suda and Uchida is
explained.

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