  The numbers and types of evolved massive stars found in nearby galaxies
provide an exacting test of stellar evolution models. Because of their
proximity and rich massive star populations, the Magellanic Clouds have long
served as the linchpins for such studies. Yet the continued accidental
discoveries of Wolf-Rayet (WR) stars in these systems demonstrate that our
knowledge is not as complete as usually assumed. Therefore, we undertook a
multi-year survey for WRs in the Magellanic Clouds. Our results from our first
year (reported previously) confirmed nine new LMC WRs. Of these, six were of a
type never before recognized, with WN3-type emission combined with O3-type
absorption features. Yet these stars are 2-3 magnitudes too faint to be WN3+O3
V binaries. Here we report on the second year of our survey, including the
discovery of four more WRs, two of which are also WN3/O3s, plus two "slash"
WRs. This brings the total of LMC WRs known to 152, 13 (8.2%) of which were
found by our survey, which is now 60% complete. We find that the spatial
distribution of the WN3/O3s are similar to that of other WRs in the LMC,
suggesting that they are descended from the same progenitors. We call attention
to the fact that five of the 12 known SMC WRs may in fact be similar WN3/O3s
rather than the binaries they have often assumed to be. We also discuss our
other discoveries: a newly found Onfp-type star, and a peculiar emission-line
object. Finally, we consider the completeness limits of our survey.
