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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Information-theoretic analysis of TNG50 simulations finds high mutual information (0.4-0.8) between bar and spiral parameters and comparable transfer entropy (0.33-0.42) in both directions, indicating mutual co-regulation.
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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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Co-evolution of bar and spiral arms in TNG50 simulations using Information Theory
Information-theoretic analysis of TNG50 simulations finds high mutual information (0.4-0.8) between bar and spiral parameters and comparable transfer entropy (0.33-0.42) in both directions, indicating mutual co-regulation.