Abstract
Using the convection model of Kuhfuß (1986) [1] the timedependence as well as the nonlocal character of the model are investigated in detail. The timedependence is studied within a one-zone model for variable stars. Nonlocality leads to a consistent description of overshooting including the influences on the temperature gradient.
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References
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Kuhfuß, R. (1987). Studies of non-local and time-dependent convection. In: Hillebrandt, W., Kuhfuß, R., Müller, E., Truran, J.W. (eds) Nuclear Astrophysics. Lecture Notes in Physics, vol 287. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0016583
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DOI: https://doi.org/10.1007/BFb0016583
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