G. A. Wade
Published 2014-09-22Version 1
We develop the requirements and potential of spectropolarimetry as applied to understanding the physics of massive stars during the immediate, intermediate-term and long-term future.
Comments: Proceedings of IAUS 307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry
Magnetic fields in massive stars, their winds, and their nebulae
Environments of massive stars and the upper mass limit
Protostellar Outflows and Radiative Feedback from Massive Stars
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