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Molecular Masers as Probes of the Dynamic Atmospheres of Dying Stars

Published onMay 31, 2019
Molecular Masers as Probes of the Dynamic Atmospheres of Dying Stars
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Abstract

The atmospheres of mass-losing red giants are characterized by the interplay between complex and dynamic processes. In the coming decade, observations of the molecular masers in the outflows of evolved stars with ultra-high angular resolution using VLBI are poised to provide groundbreaking insights into the physics of late-stage stellar mass-loss.

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