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JWST Reveals Carbon-rich Chemistry in a Transitional Disk

  • Authors: M. Volz, C. C. Espaillat, C. V. Pittman, S. L. Grant, T. Thanathibodee, M. McClure, B. Tabone, N. Calvet, F. M. Walter

M. Volz et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

The 13.6–17.7 μm range of the GM Aur spectrum. The continuum-subtracted JWST-MIRI data (black, top panel) is overlaid with the total modeled emission (red, top panel) from molecules (bottom panel) H2O (blue) and OH (pink). Slab model fits were also performed for HCN, C2H2, 12CO2, 13CO2, and 13C12CH2; however, H2O and OH were the only positive detections, while the remaining species did not match our detection criteria (see Section 3.1). The detected bright H I, H2, and atomic emission lines are labeled with dashed lines.

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