S-factor of reaction at low-energies

The astrophysical S-factor of the $$ reaction has been studied at range of bombarding energy 1-1.30 MeV. The $$ process is important in low energy astrophysics so that a possible source of energy in massive stars which have spent their hydrogen cycle. Using the Wood-saxon potential model, we have been calculated non resonances the astrophysical S-factors for the $$ transition and our results for $$  MeV is $$  MeV.b where from experimental is measured to $$ is $$  MeV.b (Couch et al., 1971) that in comparison with our data good agreement is achieved for the astrophysical S-factor of this process.