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Imaging molecular gas in high redshift galaxies at ≤1 kpc resolution

Published onMay 31, 2019
Imaging molecular gas in high redshift galaxies at ≤1 kpc resolution
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Abstract

Imaging the cool molecular gas in distant galaxies, the fuel for star formation, at ≤ 1 kpc resolution, is a prerequisite for future 'precision galaxy formation studies', addressing such basic issues as a Universal 'star formation law', cloud evolution and feed-back, and the dynamics and physical conditions in the cold gas in early galaxies.

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