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Paper: Testing a Modified Mixing-Length Theory: Comparison to the Pulsation of AGB Stars
Volume: 445, Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants
Page: 183
Authors: Wood, P.; Arnett, D.
Abstract: Pulsation models of AGB stars have been created with standard mixing-length theory and with a modified version described by Arnett et al. (2010). The modified version of the mixing-length theory gives a better reproduction of the stability and periods of AGB stars than the standard theory.
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