Individual projects:IP1: Dust formation and evolution in supernova ejecta and remnants IP2: Millimetre and submillimetre observations of dust and molecules in supernova young remnants IP3: Supernova produced radionuclides and trace elements studied by AMS IP4: The use of AMS for isotopic analysis of pre-solar materials and for the search of SN-produced r-process nuclides 182Hf and 244Pu IP5: Nucleosynthesis in stars: from nuclear physics inputs to abundances in cosmic dust Associate partners:AP1: Isolation of presolar materials for AMS analysis. Modelling of r-process nucleosynthesis |