The Program is being assembled from the contributions offered by participants, by the organizing team, in early May2001.

Program Components:

• Stellar Structure in Massive and Giant Stars
• Core-Collapse SN Models and Nucleosynthesis
• The s- and r-Process
• Bolometric Light Curves of Type II Supernovae
• Novae and 22Na and 26Al
• Gamma-Ray Lines from 44Ti, 26Al, ...; Positron Annihilation Radiation
• Chemical Evolution
• Grains and their Back-Tracing to Novae, r/s-Process etc
• Dust Formation in Wolf-Rayet Stars, Supernovae
• Supernova Remnants and their Early Evolution
• Cosmic Ray Acceleration and Supernova Remnants
• Instruments for Detection of Cosmic Radioactivities
• Instruments for Laboratory Analyses of Isotopic Compositions