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We present photoelectric and spectral observations of a hot candidateproto-planetary nebula - early B-type supergiant with emission lines inspectrum - IRAS 19336-0400. The light and color curves display fast irregularbrightness variations with maximum amplitudes dV=0.30 mag, dB=0.35 mag, dU=0.40mag and color-brightness correlations. By the variability characteristics IRAS19336-0400 appears similar to other hot proto-planetary nebulae. Based onlow-resolution spectra in the range lambda 4000-7500 A we have derived absoluteintensities of the emission lines H_alpha, H_beta, H_gamma, [SII], [NII],physical conditions in gaseous nebula: n_e=10^4 cm^{-3}, T_e=7000 \pm 1000 K.The emission line H_alpha, H_beta equivalent widths are found to beconsiderably variable and related to light changes. By UBV-photometry andspectroscopy the color excess has been estimated: E(B-V)=0.50-0.54. Jointphotometric and spectral data analysis allows us to assume that the starvariability is caused by stellar wind variations.

Variability of Hot Post-AGB Star IRAS 19336-0400 in the Early Phase of its Planetary Nebula Ionization