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Nonlinear models of pulsation and mass loss
Authors:S Höfner  M U Feuchtinger
Institution:(1) Inst. f. Astronomie d. Univ. Wien, Türkenschanzstr. 17, A-1180 Wien, Austria
Abstract:We briefly discuss the current status of our radiation-hydrodynamical models of pulsation in various stellar objects and of dust-driven mass loss in LPVs. We emphasize the importance of a future combined modelling of pulsation and mass loss in AGB stars which has to be based on reliable physical and numerical methods.
Keywords:pulsation  mass loss  dust  long period variables  AGB stars
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