Fig. 5.
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Cha Hα 1 spectrum, with the JWST-MIRI continuum subtracted data (black) compared to the stacked emission from the slab models for C2H2 + 13CCH2, HCN, CO2 + 13CO2, C6H6, C3H4, C4H2, C2H4, C2H6, CH4, H2O, and CH3. The parameters of the slab models shown can be found in Tables 2 and C.1. The H2 lines are also marked. Horizontal lines represent the windows in which the χ2 for each fitting has been evaluated. We note that the y axis is different for each panel.
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