SIMBAD references

We present uniformly reduced and measured equivalent widths, FWHM and observed line fluxes for 94 "single" WR stars (34 galactic WN, 22 galactic WC, 31 LMC WN and 7 LMC WC) based on the archive IUE spectra of WR stars gathered from different observational runs and from different epochs. The spectra are used for spectral classification in the ultraviolet region and for searching correlations among the strength and widths of emission lines of different ions. Some correlations with optical and near IR lines observed by other authors are given as well. The set of spectra we use is almost complete to 12 magnitude and representative according to spectral subtype of WR stars.