JINA - Virtual Journal of Nuclear Astrophysics,
4 November 2016
Volume 14, Issue 45 (23 Articles)
- # 8 - The impact of the revised $^{17}$O$(p,alpha)^{14}$N reaction rate on $^{17}$O stellar abundances and yields. (arXiv:1611.00632v1 [astro-ph.SR])
- O. Straniero, C.G.Bruno, M. Aliotta, A. Best, A. Boeltzig, D. Bemmerer, C. Broggini, A. Caciolli, F. Cavanna, G.F. Ciani, P. Corvisiero, S. Cristallo, T. Davinson, R. Depalo, A. Di Leva, Z. Elekes, F. Ferraro, A. Formicola, Zs. Fülöp, G. Gervino, A. Guglielmetti, C. Gustavino, G. Gyürky, G. Imbriani, M. Junker, R. Menegazzo, V. Mossa, F.R. Pantaleo, D. Piatti, L. Piersanti, P. Prati, E. Samorjai, F. Strieder, T. Szucs, M.P. Takács, D. Trezzi
- http://arxiv.org/abs/1611.00632
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
