[en] A version of the pre-equilibrium dipole γ emission account on the basis of the exciton model is suggested. The γ spectra from the (n,γ) reaction on the ⁹³Nb, ¹³³Cs, ¹⁵⁹Tb nuclei at the proton energy of 14.1 MeV are calculated. The influence of the model parameters on the calculation results is investigated. The account of the pre-equilibrium γ emission results in a large increase of the number of hard γ quanta. The satisfactory description of low-energy part of γ spectrum of radiative neutron capture was obtained as opposed to equilibrium statistic direct and half-direct models