Beryllium and Boron Evolution in the Galaxy
We present a model for the evolution of the light-nuclide abundances in the Galaxy, aimed especially at interpreting the observed beryllium and boron abundances as a function of that of iron. We present two models, one for the Galactic halo and the other for the Galactic disk. The main characteristics of the halo model are (1) the relatively rapid
Casuso, E. et al.
Fecha de publicación:
1
1997