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
An updated Nautilus code reproduces experimental steady-state [H2O2]/[H2O] and [O3]/[O2] abundance ratios in proton-irradiated ices via chemical parameter tuning, but underpredicts the fluence needed and overestimates H2O loss.
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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Simulation of proton radiolysis of H2O and O2 ices with the Nautilus code
An updated Nautilus code reproduces experimental steady-state [H2O2]/[H2O] and [O3]/[O2] abundance ratios in proton-irradiated ices via chemical parameter tuning, but underpredicts the fluence needed and overestimates H2O loss.