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Behaviour of Microturbulence with Evolution
Published online by Cambridge University Press: 30 March 2016
Extract
It is reasonable to suppose that the state of the convective zone underlying the atmosphere of cool stars correlates with the atmospheric kinematics. Following Iben (1967), as a star evolves from the red giant tip to the helium burning core phase, the convection rapidly decreases. Then the microturbulence can be expected to decrease too.
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- Copyright © Reidel 1977
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