Context. The infrared ro-vibrational emission lines from organic molecules in the inner regions of protoplanetary disks are unique probes of the physical and chemical structure of planet-forming regions and the processes that shape them. These observed lines are mostly interpreted with local thermal equilibrium (LTE) slab models at a single temperature.
No takes yet. Share an insight, caveat, or question.
A 2017 study studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: