Radiative p 16O Capture at Astrophyiscal Energies

Within the framework of the modified potential cluster model with forbidden states and classification of states according to the Young tableaux, the possibility is considered of describing experimental data for the astrophysical S-factor of radiative p16O capture to the ground state of the 17F nucleus. It is shown that on the basis of E1 transitions from p16O scattering states to the ground state of 17F in the p16O channel overall success is achieved in explaining the magnitude of the measured cross sections at astrophysical energies.