Cross-sections for nat P b(p, xn) 201−207 Bi, 204 P b(p, 1 − 4n) 201−204 Bi and 206 P b(p, 3n) 204 Bi reactions have been determined in the astrophysical energy range 20 − 30 M eV . The analysis were performed by γ-spectroscopy associated with half-lives measurements. The results were compared with previously experimental data, when available, and with theoretical calculations performed using TALYS code. We report a possible new γ transition from 204m P b and other theoretical discrepancies, probably due overestimation of the Coulomb barrier and neutron binding energy. Also reported are new determinations of the energies and intensities of the γ's emitted in the decays of 205,206 Bi. We discuss possible implications for the r/rp-processes in neutrino-driven wind in supernovae and neutron stars mergers.