Updated DALI models reproduce observed C2H2 fluxes with solar C/O and find the C2H2/H2O flux ratio sensitive to elemental abundances and small-grain abundance in planet-forming disk regions.
Carbon and oxygen elemental abundances
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Thermo-chemical models predict that NH3 is undetectable with JWST-MIRI even at high N/H while NO may be detectable, and observations confirm no NH3 detections with one tentative NO in V1094 Sco.
citing papers explorer
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Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties
Updated DALI models reproduce observed C2H2 fluxes with solar C/O and find the C2H2/H2O flux ratio sensitive to elemental abundances and small-grain abundance in planet-forming disk regions.
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Detecting nitrogen-carriers in the inner regions of protoplanetary disks
Thermo-chemical models predict that NH3 is undetectable with JWST-MIRI even at high N/H while NO may be detectable, and observations confirm no NH3 detections with one tentative NO in V1094 Sco.