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Imaging Entire Molecular Clouds in many Lines: Formation of Stars and Planets

Published onMay 31, 2019
Imaging Entire Molecular Clouds in many Lines: Formation of Stars and Planets
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Abstract

Studies of molecular line emission at >70 GHz will substantially advance our picture of how stars from in the molecular clouds of the Milky Way. Such work requires spatially resolved imaging of entire clouds at ~0.1 pc resolution. This work requires both small and large telescopes, as well as ALMA.

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