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The Current State of Stellar Mixing-Length Theory
Published online by Cambridge University Press: 15 February 2018
Summary
The basic assumptions of the mixing-length formalism are described, and the theory is developed with a view to representing convection in stars. Directions in which the results might be improved and extended are indicated.
- Type
- I. Mixing-Length Theory
- Information
- International Astronomical Union Colloquium , Volume 38: Problems of Stellar Convection , 1977 , pp. 15 - 56
- Copyright
- Copyright © 1976