Image Details
Caption: Figure 10.
Emission-line luminosities (left) and emitting masses (right) integrated from slab model fits to C2H2, HCN, and CO2 between 12 and 16 μm in JDISCS sources. Despite spanning a limited range in stellar masses, the targets display at least an order of magnitude variation in mid-infrared luminosity and mass of each molecule. Violin widths represent the number of disks with detections of each molecule, such that narrower violins correspond to lower detection rates.
© 2025. The Author(s). Published by the American Astronomical Society.