Spectropolarimetry of massive stars: Requirements and potential from today to 2030
G.A. Wade
TL;DR
This paper discusses the current and future capabilities of spectropolarimetry in studying massive stars, outlining necessary requirements and potential scientific advancements from now until 2030.
Contribution
It defines the requirements and explores the potential of spectropolarimetry for advancing understanding of massive star physics over the next decade.
Findings
Identifies key technological requirements for future spectropolarimetric instruments.
Highlights potential scientific breakthroughs in massive star physics.
Provides a roadmap for spectropolarimetry development from now to 2030.
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.
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