Radiative <i>р</i><sup>14</sup>N-capture to second and fifth exited states of <sup>15</sup>O
The description results were obtained for available experimental data on astrophysical S-factor of the proton capture on 14N reaction to second and fifth exsited states of 15O at 5.24 and 6.86 MeV with J = 5/2+ at proton energy up to 1 MeV in the frame of modified potential cluster model. Supposing that these exsited states are D5/2-levels, and two resonanses at 260 and 987 keV are D-scattering waves, it is possible to reproduce experimental data for S-factor good. The calculations were done in the energy range from 30 keV.