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Unlocking the Secrets of Late-Stage Stellar Evolution and Mass Loss through Radio Wavelength Imaging

Published onMay 31, 2019
Unlocking the Secrets of Late-Stage Stellar Evolution and Mass Loss through Radio Wavelength Imaging
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Abstract

Many details concerning the physics of late-stage stellar mass loss remain poorly understood. Observations at cm, mm, and sub-mm wavelengths that resolve the radio surfaces and extended atmospheres of evolved stars in space, time, and frequency are poised to provide groundbreaking new insights into these questions in the coming decade.

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