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The Evolution of Rapidly Rotating B/Be Stars
Published online by Cambridge University Press: 14 August 2015
Abstract
Rotation can significantly change the moment-of-inertia of a main sequence star. As a result, the ZAMS rotation rate need only be within ~30% of the critical value in order to reach critical rotation during the hydrogen burning stage. Calculations of the evolution of rotating stars show that the Be stars result from a normal (Maxwellian) distribution of B-star rotation velocities.
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- V. Rotation and Binarity
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- Copyright © Reidel 1982
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