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Observations Bearing on the Theory of Stellar Convection II

Published online by Cambridge University Press:  15 February 2018

Erika Böhm-Vitense
Erika Böhm-Vitense*
Affiliation:
University of Washington, Seattle, Wa., U.S.A., and University of Göttingen, Germany

Summary

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It is shown that the best way to get information about efficiency of convective energy transport in the hydrogen convection zones in stars other than the sun is presently contained in continuous energy distributions of A and F stars. Scans show that convective energy transport must be much more efficient than thought hitherto. The scans indicate that rapid rotation enhances convective energy transport.

Figure 1 lists all the observations, we could think of, which are influenced by the outer convection zone and which can therefore give us information for our convection theory.

Type
I. Mixing-Length Theory
Information
International Astronomical Union Colloquium , Volume 38: Problems of Stellar Convection , 1977 , pp. 63 - 86
Copyright
Copyright © 1976

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