Spectropolarimetry of massive stars: Requirements and potential from today to 2030
arXiv:1409.6353 · doi:10.1017/S1743921314007431
Abstract
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.
arXiv commentProceedings of IAUS 307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry
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