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HII Regions and the Warm Ionized Medium

Published onMay 31, 2019
HII Regions and the Warm Ionized Medium
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Abstract

Plasma of temperature 10,000K is created by OB stars and takes the form of discrete HII regions and diffuse gas. It is the key to determining the impact of massive stars on the interstellar medium (ISM) and the lifecycle of ISM gas. We review research this plasma, highlight outstanding questions, and provide recommendations for future facilities.

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