Abstract
Pulsation models of AGB stars have been created with standard mixinglength theory and with a modified version described by Arnett et al. (2010). The modi-fied version of the mixing-length theory gives a better reproduction of the stability and periods of AGB stars than the standard theory.
| Original language | English |
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| Title of host publication | Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants: Proceedings |
| Editors | F. Kerschbaum, T. Lebzelter, and R.F. Wing. San Francisco |
| Place of Publication | San Francisco, United States |
| Publisher | Astronomical Society of the Pacific |
| Pages | 183-184pp |
| Edition | Not Peer Reviewed |
| ISBN (Print) | 9781583817704 |
| Publication status | Published - 2011 |
| Event | Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants - Vienna, Austria, Australia Duration: 1 Jan 2011 → … |
Conference
| Conference | Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants |
|---|---|
| Country/Territory | Australia |
| Period | 1/01/11 → … |
| Other | August 16-20 2010 |