  The possibility of description of the experimental data for the astrophysical
S-factor of the radiative proton capture on 15N at the energies from 50 to 1500
keV was considered in the framework of the modified potential cluster model
with the classification of the orbital states according to Young tableaux. It
was shown that, on the basis of the M1 and the E1 transitions from different
states of the p15N scattering to the ground state of 16O in the p15N channel,
it is quite succeed to explain general behavior of the S-factor in the
considered energy range in the presence of two resonances.
