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AGB star models. Results from 1D stellar evolution and multi-dimensional hydrodynamics simulations

Published online by Cambridge University Press:  01 April 2008

Falk Herwig
Falk Herwig*
Affiliation:
Keele Astrophysics Group, School of Physical and Geographical Sciences, Keele University, Staffordshire ST5 5BG, UK email: fherwig@astro.keele.ac.uk
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Abstract

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In this review I am discussing the current state of simulating the internal evolution of AGB stars. Recent work on AGB stars include the effect of rotation, magnetic fields and internal gravity waves, as well as thermohaline mixing induced by the 3He + 3He pp-chain reaction. Hydrodynamic simulations of the interior convection of AGB stars are now becoming available, giving insights to convective boundary mixing, for example for He-shell flash convection. At very low metallicity convective-reactive events are encountered in AGB stars (as well as in massive stars), and the necessity of hydrodynamic simulations to address this difficult phase of stellar evolution is emphasized.

Keywords

Stars: AGB and post-AGBstars: rotationstars: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S252: The Art of Modeling Stars in the 21st Century , April 2008 , pp. 205 - 213
Copyright
Copyright © International Astronomical Union 2008

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