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Stellar physics with high-resolution UV spectropolarimetry

Published onMay 31, 2019
Stellar physics with high-resolution UV spectropolarimetry
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Abstract

Current burning issues in stellar physics, for both hot and cool stars, concern their magnetism and its impact on stellar structure, evolution, activity, and circumstellar environment. However, the role of magnetism is complex and thus poorly understood as of today. It needs to be quantified with high-resolution UV spectropolarimetric measurements.

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