Testing a Modified Mixing-Length Theory: Comparison to the Pulsation of AGB Stars

Details Testing a Modified Mixing-Length Theory: Comparison to the Pulsation of AGB Stars Testing a Modified Mixing-Length Theory: Comparison to the Pulsation of AGB Stars

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445..183w&link_type=abstract

Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca

Astronomy and Astrophysics

Astronomy

1

Scientific paper

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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