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As part of our ongoing Wolf-Rayet (WR) Magellanic Cloud survey, we havediscovered 13 new WRs. However, the most exciting outcome of our survey is notthe number of new WRs, but their unique characteristics. Eight of ourdiscoveries appear to belong to an entirely new class of WRs. While one mightnaively classify these stars as WN3+O3V binaries, such a pairing is unlikely.Preliminary CMFGEN modeling suggests physical parameters similar to early-typeWNs in the Large Magellanic Cloud except with mass-loss rates three to fivetimes lower and slightly higher temperatures. The evolution status of thesestars remains an open question.

The Discovery and Physical Parameterization of a New Type of Wolf-Rayet Star