A Modern Search for Wolf-Rayet Stars in the Magellanic Clouds. IV. A Final Census
Kathryn F. Neugent, Philip Massey, and Nidia Morrell

TL;DR
This four-year survey of the Magellanic Clouds identified new Wolf-Rayet and Of-type stars, discovered a new class called WN3/O3s, and provided an updated catalog, challenging previous claims about their isolation.
Contribution
The paper presents the discovery of a new Wolf-Rayet subclass, WN3/O3s, and offers a comprehensive, updated catalog of LMC WR stars with revised data and analysis of their spatial distribution.
Findings
Discovered 15 new WRs and 12 Of-type stars.
Identified a new WR subclass, WN3/O3s.
Found WN3/O3s are spatially distributed like other massive stars.
Abstract
We summarize the results of our four year survey searching for Wolf-Rayet (WR) stars in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). Over the course of this survey we've discovered 15 new WRs and 12 Of-type stars. In this last year we discovered two rare Of-type stars: an O6.5f?p and an O6nfp in addition to the two new Of?p stars discovered in our first year and the three Onfp stars discovered in our second and third years. However, even more exciting was our discovery of a new type of WR, ones we are calling WN3/O3s due to their spectroscopic signatures. We describe the completeness limits of our survey and demonstrate that we are sensitive to weak-lined WRs several magnitudes fainter than any we have discovered, arguing that there is not a population of fainter WRs waiting to be discovered. We discuss the nature of the WN3/O3s, summarizing the results of our…
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