PI: Daniel Bemmerer and Antonio Caciolli

WG members: D. Bemmerer, C. Broggini, A. Caciolli, F. Cavanna, R. Depalo, Z. Elekes, F. Ferraro, G. Gervino, A. Guglielmetti, I. Kochanek, P. Marigo, R. Menegazzo, D. Piatti, P. Prati, O. Straniero, T. Szuecs, M. Takacs, D. Trezzi

 

Astrophysical Motivation:

  •  AGB stars

  • competing with 22Ne(α, n)25Mg for s- process

  • goal: measurement of the 395 keV resonance strength 

 

Documentation