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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4 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 4representative citing papers
Galaxy interactions at z~5 trigger star-formation bursts responsible for ~42% of stellar mass growth, half from new stars formed during the interaction.
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.
citing papers explorer
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Molecular Gas Structure and Star Formation Diversity in Stephan's Quintet Revealed by ACA CO(1-0) Mapping
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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Interaction-induced star formation boosts stellar mass assembly in $z\sim5$ galaxies
Galaxy interactions at z~5 trigger star-formation bursts responsible for ~42% of stellar mass growth, half from new stars formed during the interaction.
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Metal-Poor Gas Accretion Drives Giant Clump Formation at 0.6 < z < 2.6
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.