Figure 2. Detection of C6H6 (benzene), CO2, and C4H2. Continuum subtracted MIRI spectrum, showing a zoom-in on a number of key molecular transitions in the 14.7-16 µm region (top panel) and their best fit slab models assuming an emitting area of π (0.07au)2 (bottom panel). Use mouse to zoom-in.

Tabone et al., arXiv:2304.05954 [astro-ph.EP]