A Simplified Local Mixing-Length Theory with Helium Flux and without Radiative Heat Loss from the Convective Element

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概要

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• 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.SemiconvectionMixing-length theory of convection

• 東北大学の論文
• 1990-02-28

著者

• Umezu Minoru

  Astronomical Institute Faculty Of Science Tohoku University

関連論文

• On the Models of Early Main Sequence Evolution of Moderately Massive Stars with growing Inhomogeneous Convection Zone
• A Simplified Local Mixing-Length Theory with Helium Flux and without Radiative Heat Loss from the Convective Element

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