First large-scale ACA CO(1-0) map of Stephan's Quintet identifies molecular gas structures and a negative SFE-velocity dispersion correlation, implying turbulence regulates star formation in this interacting group.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Clumpy galaxies at cosmic noon show systematically lower metallicities than the mass-metallicity relation, with clump properties indicating metal-poor gas accretion as the driver rather than mergers.