Spectral and photometric observation of sg B[e] MWC 314 star

In the paper spectrophotometric and photometric data, received for sg B[e] MWC 314 star during 2001-2004 years at high mounting Assy-Turgen observatory are given. In spectra the Hα, Hβ, HeI, numerous FeII intensity lines and forbidden [NII], [OI] lines are presented. The variety of Hα lines intensity relatively to continuum (from 24 to 33) is observed. For this time the Hα line equivalent width EW is changed in the limits 138-179 Angstrom, the brightness in range V=9,m82-9.m96; (B-V)=1.m77-1.m82; (V-R)=1.m53-1.m64. There are the distinct correlation's of Hα line equivalent width EW with star colour index (B-V): at the increasing of EW the (B-V) colour index is increased. (author)