How does rotation change the radius of a low mass stellar model

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Models, Radii, Stellar Rotation, Stellar Structure, Angular Velocity, Stellar Envelopes, Stellar Mass

Scientific paper

The results of different authors for stellar model computations of
chemically homogeneous stars of one solar mass in uniform rotation do
not agree near breakup velocity. It is shown that the differences can be
explained from the approximation used for the convective envelope. Some
qualitative arguments can be given to support the numerical results.

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