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Paper: Small and intermediate mass stellar evolution - Main sequence and close to it
Volume: 40, Inside the Stars, IAU Colloquium 137
Page: 410
Authors: Noels, A.; Grevesse, N.
Abstract: We present the standard models for small and intermediate main sequence stars and we discuss some of the problems arising with semiconvection and overshooting. The surface abundance of Li serves as a test for other physical mechanisms, including microscopic and turbulent diffusion, rotation and mass loss.
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