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We report the discovery of two new Wolf-Rayet (WR) galaxies: Mrk~1039, andF08208$+$2816. Two broad WR bumps at 5808\AA~ and 4650\AA~ indicate thepresence of WCE and WNL star population in all two sources. We also confirm thepresenceof WR features in Mrk~35, previously detected in a different position.The observed equivalent width of the WR bump at 4650\AA~ and the derived numberratios of WR/(WR$+$O) imply that star formation in these sources takes placeinshort burst duration. Comparisons with the recent models of WR populations inyoung starbursts with the observed EW(\HeII)/EW(\CIV)/EW(WRbump) and theirrelative intensitie provide an indication that the stellar initial massfunction in some WR galaxies might not be Salpeter-like. It is interesting tofind that the luminous IRAS source, F08208$+$2816, has little dust reddening,probably because of the existence of a powerful superwind. By comparisons withother starbursts observed with the Hopkins Ultraviolet Telescope, F08208$+$2816as a merging system renders a chance to study the contribution from youngstarbursts to the UV background radiation in universe.Comment: 22 pages, 6 figures, 4 tables, accepted by The Astrophysical Journa

New Wolf‐Rayet Galaxies with Detection of WC Stars