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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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