Spatially resolved NOEMA observations reveal extended molecular gas disks in main-sequence galaxies at z=1.1-1.6, supporting steady accretion via spirals or bars instead of merger-driven starbursts.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2representative citing papers
The high-contrast dust asymmetry in HD 34700A is reproduced by a vortex model, with contrast levels excluding eccentric cavity orbit clustering.
citing papers explorer
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NOEMA3D: Spatially resolved dust, CO, and [C I] in massive star-forming main sequence galaxies at cosmic noon
Spatially resolved NOEMA observations reveal extended molecular gas disks in main-sequence galaxies at z=1.1-1.6, supporting steady accretion via spirals or bars instead of merger-driven starbursts.
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The Circumbinary Disc of HD 34700A II. Analysis of a strong dust asymmetry
The high-contrast dust asymmetry in HD 34700A is reproduced by a vortex model, with contrast levels excluding eccentric cavity orbit clustering.