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Stellar Feedback in the ISM Revealed by Wide-Field Far-Infrared Spectral-Imaging

Published onMay 31, 2019
Stellar Feedback in the ISM Revealed by Wide-Field Far-Infrared Spectral-Imaging
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Abstract

Atomic and molecular far-IR ( ~30 to 350 microns) lines are the most sensitive probes of stellar feedback processes. They allow us to quantify the deposition and cycling of energy in the ISM. In this white paper we emphasize the need of a space telescope with wide-field spectral-imaging capabilities in the critical far-IR domain.

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