  The possibility of description of the experimental data for the astrophysical
S-factor of the proton radiative capture on 16O to the ground and first excited
states of 17F was considered in the frame of the modified potential cluster
model with forbidden states and classification of the states according to Young
tableaux. It was shown that on the basis of the E1 transitions from the P
states of p16O scattering to the bound states of 17F in the p16O channel, it
generally succeed to explain the value of measured astrophysical S-factors and
reaction rates at astrophysical energies.
