Philip Massey, Kathryn F. Neugent, Emily M. Levesque
Published 2017-06-08Version 1
The nearby galaxies of the Local Group can act as our laboratories in helping to bridge the gap between theory and observations. In this review we will describe the complications of identifying samples of OB stars, yellow and red supergiants, and Wolf-Rayet stars, and what we have so far learned from these studies.
Comments: To appear in Philosophical Transactions A, from the conference "Bridging the Gap: from Massive Stars to Supernovae."
The MiMeS Survey of Magnetism in Massive Stars
The Infrared Properties of Massive Stars in the Magellanic Clouds
Environments of massive stars and the upper mass limit
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