Аннотация:The spectral energy distribution in the continuum of Pleione from lambda 3200 A to lambda 7600 A in erg/cm2 sec.A, and equivalent widths for hydrogen lines H (alpha)- H (sigma) given in tables were measured on the base of the observations with low resolution spectrometers at the Crimean laboratory of the Sternberg Astronomical Institute during 1972 - 1989. The energy distribution is analysed by means of Gorbatsky method for purpose of obtaining information about effective temperature of stellar envelope. When the envelope is considered as opitcaly thin for the Balmer continuum radiation we obtained T(eff) 11500 - 12500 K, Te 8000 - 10000 K and Ne (3-12)*10^11 cm^-3.