  As part of our ongoing Wolf-Rayet (WR) Magellanic Cloud survey, we have
discovered 13 new WRs. However, the most exciting outcome of our survey is not
the number of new WRs, but their unique characteristics. Eight of our
discoveries appear to belong to an entirely new class of WRs. While one might
naively classify these stars as WN3+O3V binaries, such a pairing is unlikely.
Preliminary CMFGEN modeling suggests physical parameters similar to early-type
WNs in the Large Magellanic Cloud except with mass-loss rates three to five
times lower and slightly higher temperatures. The evolution status of these
stars remains an open question.
