PI: Marialuisa Aliotta

WG members: M Aliotta, A Best, CG Bruno, T Davinson, A Formicola, Zs Fulop, G Gervino, A Guglielmetti, G Gyurky, G Imbriani, M Junker, F Strieder, D Trezzi, T Szuecs

 

Astrophysical Motivation:

  • 18O burning in AGB stars

  • 15N abundance in SiC grains

  • 19F nucleosynthesis in AGB stars

 

Documentation