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Methanol Emission Tracing Ice Chemistry and Dust Evolution in the TW Hya Protoplanetary Disk

  • Authors: John D. Ilee, Catherine Walsh, Jenny K. Calahan

John D. Ilee et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 11.

Column density of gas-phase methanol (CH3OH) at a radius of 100 au for the canonical elemental abundances (C/O = 0.43; O/H = 3.2 × 10−4), and two models where oxygen is globally depleted by factors of 10 and 100 and C/O is set to 2. Shown are the results for the models with grain-surface chemistry, reactive desorption, and fractal grains, and with (GR+RD+FR+D2G) and without (GR+RD+FR) ice-to-gas mass scaling.

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