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Physical Conditions in the Cold Gas of Local Galaxies

Published onMay 31, 2019
Physical Conditions in the Cold Gas of Local Galaxies
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Abstract

We describe a next major frontier in studies of galaxy evolution and star formation: linking physical conditions in the cold, star-forming interstellar medium to host galaxy and local environment. The key observations will be cm-, mm-, and submm-wave spectroscopy and spectroscopic imaging. We highlight key paths for progress in the next decade.

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