Abstract
D01 Laboratory Studies on Presolar Grains from AGB Stars D02 Fe II and [Fe II] Emission Lines as a Diagnostic Tool to Probe the Shocked Atmospheres of M-type Miras D03 Long Term Modelling of Mass Loss on the Late AGB D04 The Role of AGB Stars in Galactic Chemical Evolution D05 Nucleosynthesis and Massive Stars in the Orion Region D06 The Shapes of Gamma-Ray Lines from Radioactives – Prospects for INTEGRAL D07 Dynamical Atmospheres and Winds of AGB Stars D08 Tracing AGB s-process Nucleosynthesis by the Analysis of Post-AGB Stars D09 Nuclear Astrophysiscs in AGB Stars D10 Microphysical Aspects of Dust Formation in the Winds of AGB Stars D11 Three-component Modeling of AGB Star Winds D12 The Surface Composition of Hydrogen-deficient Post-AGB Stars D13 The s Process in AGB Stars from the Nucleosynthesis Point of View
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